The galaxy presents a generally smooth, elliptical morphology. It exhibits a somewhat elongated, cigar-like shape. A bright central bulge is noticeable, surrounded by a fainter, more diffuse halo. There appears to be some asymmetry or minor disturbance present, possibly indicative of a weak tidal interaction or past minor merger event. The color gradient suggests a population of older stars, with a hint of ongoing star formation. There are no obvious spiral arms or significant dust lanes visible in this image.
