The galaxy appears to be a relatively compact object, exhibiting a generally elliptical morphology. There is evidence of a central bright region that transitions into a fainter, more diffuse halo or disk. The color profile suggests potential radial variations in stellar populations, with bluer colors concentrated in the central region and potentially redder colors in the outskirts. There might be some minor disturbances, possibly suggestive of interactions or past merger events. The main body of the galaxy is relatively smooth, with no obvious spiral arm structure or large-scale features visible. The overall impression is that of a galaxy that may have undergone some past dynamical activity, though appears generally relaxed.
