The object presents as a single, though morphologically complex, galaxy. A dominant, smooth, and highly luminous spheroid is evident, exhibiting a concentrated central bulge. The color is generally yellowish-orange, suggestive of an older stellar population. 

Extending from this main body is a fainter, bluish structure. This appears less centrally condensed and exhibits a more diffuse morphology. The color indicates the presence of younger, hotter stars. The overall impression is of a possible interaction or merger event, with one component having a more disk-like feature. There are some indications of tidal tails or debris extending from the main body as well, indicating ongoing or past gravitational interaction.
