The galaxy presents as a centrally concentrated object with a generally smooth appearance. The light distribution is centrally condensed, exhibiting a high degree of radial symmetry. There's very little evidence of spiral arm structure. The galaxy appears elliptical or lenticular, with a dominant, rounded central bulge. There is a subtle color gradient moving from the center outwards. The core is a brighter, whiter hue, suggesting an older stellar population. The outer edges are somewhat bluer, indicating the presence of a younger stellar population. The overall morphology suggests a galaxy that is likely in a relatively late stage of its evolution, possibly having undergone past merger events that have smoothed out any prominent features. There is no indication of strong tidal features or ongoing major mergers. The colors suggest a moderate level of recent star formation, with the lack of clear spiral arms indicating the star formation is not organized in the disk like structures.
