The galaxy presents as a flattened elliptical or lenticular morphology. The central region exhibits a pronounced bulge, characterized by a smooth, concentrated distribution of light, appearing yellowish-orange in color, suggestive of an older stellar population. Surrounding the bulge, a fainter, more diffuse disk-like structure is subtly visible. Within the disk, there is little indication of spiral arm structure. The smoothness of the galaxy indicates a relatively quiescent star formation rate and a well-mixed stellar population. A slight asymmetry is observed in the outer regions, potentially indicating a past or ongoing minor interaction or disturbance. Overall, the galaxy gives the impression of being a evolved system with minimal ongoing star formation.
