The galaxy presents a generally smooth and rounded morphology. The light is concentrated in a central region, potentially indicating a bulge. A fainter, diffuse extension is observed to the left of the central bulge. There is an absence of clear spiral arm structures or significant dust lanes visible within the galaxy's disk. The overall color appears reddish, suggesting an older stellar population. There do not appear to be any significant tidal features or distortions that would indicate a major merging event, though a minor disturbance may be present based on its slightly irregular shape. The galaxy may be undergoing minor interactions with the smaller region to its left.
