The galaxy presents as a relatively compact, elliptical system with a smooth, diffuse light distribution. It is characterized by a bright, concentrated central bulge that appears yellowish, suggestive of an older stellar population. The overall shape is approximately circular, showing minimal signs of significant rotational flattening. The outer regions of the galaxy gradually fade into the background, exhibiting a subtle blueish color. There is no evidence of prominent spiral arms, dust lanes, or ongoing major merging activity. Faint evidence of a minor tidal feature is present on one side of the galaxy, suggesting a possible gravitational interaction or minor merger in its past.
