The galaxy presents as a roughly elliptical structure with a smooth, diffuse light distribution. A concentrated central bulge is apparent, exhibiting a yellowish hue. The radial color profile suggests a possible redder stellar population in the core region, indicative of older stars or a higher metallicity. No distinct spiral arms or prominent dust lanes are visible. The overall shape is closer to an elliptical morphology, possibly an E3-E5 on the Hubble sequence, with only a very slight flattening. There's no clear indication of ongoing major merging events, although subtle asymmetries might suggest minor interactions. The outer regions of the galaxy gradually fade into the background, consistent with a lack of significant recent star formation in the disk.
