The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge. The color profile suggests a population dominated by older stars, as indicated by the reddish-yellow hue, particularly pronounced in the core. There is very little evidence of spiral arm structure or dust lanes. The outer regions appear diffuse and fade gradually into the background sky, suggesting a lack of active star formation in the disk. There may be subtle signs of a weak tidal interaction or minor disturbance in the morphology. The galaxy appears to be fairly isolated.
