The galaxy presents as a relatively smooth, elliptical-like structure, elongated along one axis giving it a cigar-like shape. A bright, concentrated central region is visible, suggesting a significant bulge component. The color profile indicates a yellow-red hue overall, potentially indicative of an older stellar population and lower levels of recent star formation. Faint, diffuse light extends outwards from the central region, without any immediately obvious spiral arm structures. There may be some minor disturbance or a slight irregularity in the outer halo, but it does not appear to be undergoing a major merger or disruption. The galaxy appears to be relatively isolated, with no other interacting galaxies in close proximity within the field of view.
