The galaxy presents a generally elliptical morphology, appearing largely spheroidal with a smooth light distribution. The central region displays a brighter, more concentrated intensity, suggesting a substantial stellar population and/or an active galactic nucleus. The overall color profile is relatively uniform across the galactic body with a slight color change towards the outer edges. There is a subtle color gradient, transitioning from a more yellow/red core to a slightly bluer halo, suggestive of a moderate amount of ongoing star formation within the galaxy, particularly in the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible, indicating a lack of significant ordered structure associated with disk galaxies. There is no indication of a major ongoing merger event, with the overall shape appearing mostly undisturbed. Faint hints of tidal features or minor disturbances are present, which may indicate a recent minor merger or interaction.
