This galaxy appears as a relatively small, faint blueish object. It exhibits a somewhat irregular morphology, deviating from a perfectly smooth elliptical shape. There are indications of disturbed features or possibly spiral arm segments, although the resolution limits detailed classification. The galaxy is not particularly concentrated, with a moderately diffuse light distribution, suggesting some level of ongoing or recent star formation. There is no discernible central bulge. Based on its morphology, this galaxy might be undergoing some type of interaction or experiencing internal processes that disrupt its overall structure. The light detected indicates the galaxy contains a mixture of stellar populations. The bluish color suggests the presence of young, hot stars, indicating recent star formation, and the lack of a strong red signature suggests an absence of large amounts of old stars. There is also a redder hue detected, indicating the presence of some older stars. The object does not show any clear indications of an ongoing major merger, however it is difficult to be certain based on the available image.
