The galaxy presents as a centrally concentrated structure with a relatively smooth overall appearance. The core region exhibits a bright, yellowish hue, suggestive of an older stellar population. Extending outwards from the core, there is a more diffuse, bluish component. The elongation of the galaxy suggests a somewhat flattened, disk-like structure, though the lack of clearly defined spiral arms points to a more lenticular morphology. There is no evidence of significant tidal disturbances or ongoing mergers. Faint blue regions present throughout the galaxy could suggest some star formation.
