The galaxy presents as a relatively smooth, elliptical-like structure, though it appears to have a slightly elongated, cigar-shaped morphology. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer edges. Its color index suggests a population dominated by older stars, giving it a yellowish-red hue. There is no distinct evidence of spiral arms or significant dust lanes within the visible structure, suggesting a later-type galaxy with minimal ongoing star formation. Based on the overall morphology, there is a slight indication of a minor disturbance in the galaxy's shape, possibly due to a past or ongoing interaction with a smaller object. However, there is no clear evidence of a major merger event, and the galaxy appears largely undisturbed.
