This galaxy presents as a relatively bright, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish hue, indicative of an older stellar population. Extending outward from the core, we observe a bluer disk-like structure. This suggests ongoing or recent star formation in the outer regions.

The galaxy displays a moderate level of internal disturbance. While the primary structure appears coherent, there is a subtle asymmetry and potentially signs of tidal interactions, possibly with a past or ongoing minor merger. The overall shape is elongated, leaning toward an "in between" classification between round and cigar-shaped. There is no clear indication of a strong bar structure or spiral arms, but subtle disk-like features and patchy color variations are present within the extended halo, suggesting some level of internal structure.
