The galaxy presents as an elliptical form, with a relatively high Sersic index, indicating a centrally concentrated light profile. The light is primarily concentrated in the central bulge, with a gradual decrease in intensity towards the edges. The galaxy is elongated, and the light distribution is somewhat irregular, suggesting a possible ongoing or recent merger event. There are some color variations across the galaxy, with the central region exhibiting a more yellow hue, potentially indicating an older stellar population. A bluer region to the right suggests an area of more recent star formation. There is some indication of tidal features, specifically faint, diffuse extensions, which may indicate the disruption of one or both galaxies during the merger.
