The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge that gradually fades into the outer regions. The central region appears yellowish-red, possibly indicative of an older stellar population and dust. The outer areas show a hint of greenish-blue, which may suggest the presence of younger, hotter stars and ongoing star formation, although this activity seems subdued. No distinct spiral arms or bar features are discernible. There may be a slight distortion or asymmetry in the overall shape, but it does not appear to be undergoing any major merger activity or tidal disruption.
