The galaxy presents as a relatively compact object with an apparent smooth morphology, although some faint, diffuse features are subtly visible. It appears centrally condensed with a bright, yellowish core, suggestive of an older stellar population and a potentially supermassive black hole at its center. Extending outwards from the core is a less defined, bluer region. This bluer color indicates the presence of younger, hotter stars, possibly within spiral arms or regions of ongoing star formation, although the overall smoothness suggests a disrupted spiral structure. The general roundness indicates it may be an elliptical galaxy, or a spiral galaxy that is not viewed edge-on. There is a faint suggestion of a tidal feature or minor disturbance on one side of the galaxy, indicating possible interaction with another galaxy.
