The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a diffuse halo. The color profile indicates a redder hue in the central regions, suggesting an older stellar population. There is little to no evidence of spiral arms or significant dust lanes. The overall morphology suggests a quiescent galaxy, possibly nearing the end of its star formation cycle. There may be some evidence of a tidal interaction with a smaller object nearby, but without further data it's impossible to definitively assess the merger stage. The galaxy presents a regular, well-defined shape with no pronounced distortions.
