The galaxy presents as a moderately luminous, relatively compact object with a generally elliptical morphology, though exhibiting some slight asymmetry. Its light distribution is dominated by a smooth, centrally concentrated component, which is likely an indication of an older stellar population. However, there's a suggestion of a faint disk-like structure or possible tidal arm extending from the central region. The color profile appears fairly uniform, exhibiting a modest blue tint indicative of recent or ongoing star formation activity, though this is not overwhelming. There may be some indications of a minor disturbance or interaction in the galaxy's morphology, which could be attributed to a past or ongoing minor merger event. Overall, the galaxy appears to be in a transitional stage, potentially evolving from a more actively star-forming system toward a more quiescent state.
