The galaxy presents a mostly smooth, elliptical morphology, exhibiting a relatively concentrated central bulge. The overall shape is moderately round, with a slight elongation. The central region appears bright and unresolved, indicating a high stellar density and potentially an active galactic nucleus (AGN). Surrounding the core is a fainter, more diffuse halo. There is a subtle disk-like structure but it is not particularly pronounced. The color profile suggests the presence of an older stellar population, with a redder hue dominating the galactic body, and a slight hint of blue near the central bulge. There is little evidence of spiral arms or other significant features indicative of recent major mergers.
