The galaxy presents as a roughly elliptical object, exhibiting a noticeable color gradient across its structure. A bright, concentrated central bulge dominates the morphology. Emanating from this central region, a diffuse halo extends outwards. This halo shows a slight elongation, indicating a possible disk-like structure viewed at an angle, or perhaps some past tidal interaction. 

One side of the galaxy displays a distinct extension, appearing bluer in color than the main body. This feature suggests a region of active star formation, potentially resulting from a merger or accretion event. The rest of the galaxy appears to be comprised primarily of older stars. The relatively smooth appearance of the galaxy suggests that this is either an elliptical galaxy or that it is a spiral galaxy with a high degree of central concentration and bulge dominance.
