The galaxy presents as a relatively smooth, elliptical-like structure. A concentrated central bulge is apparent with a yellowish hue, suggesting an older stellar population. The outer regions show a gradual decrease in intensity. Hints of bluer color appear closer to the central region, which suggests a region of active star formation. The galaxy appears largely undisturbed, exhibiting a generally symmetrical form with no obvious signs of tidal tails or significant distortions indicative of recent major merger activity. There may be a minor disturbance or merging event happening on the outer edges of the galaxy, but it is not causing significant distortion of the central bulge.
