The object presents as a galaxy, exhibiting a generally elliptical morphology. The light profile appears smooth and concentrated, lacking significant spiral arm structures or prominent dust lanes. A bright central bulge dominates the visual appearance, with light intensity gradually decreasing outwards from the core.

The galaxy's color appears somewhat uniform across its extent, suggesting an older stellar population with relatively low ongoing star formation. A slight color gradient may be present, transitioning from a slightly yellower hue in the core to a somewhat bluer tint in the outer regions, possibly indicating some younger stars are present in the extended disk. No distinct features indicative of recent or ongoing mergers, such as tidal tails or disrupted morphology, are readily apparent.
