The galaxy appears as a centrally concentrated object with a somewhat elongated morphology. The central region exhibits a bright, smooth distribution of light, suggesting an older stellar population or a bulge component. Fainter, more diffuse light extends outwards from the center, showing some asymmetry. There is evidence of a faint, disk-like structure, possibly exhibiting some irregularities. There is also a chance this galaxy is undergoing minor disturbance or is in the early stages of a minor merger. Star formation appears to be present, but it is not vigorous.
