The galaxy presents an elliptical morphology, though not perfectly circular. A central bulge is prominent, exhibiting a high surface brightness. The overall color gradient suggests the presence of an aging stellar population, particularly concentrated within the bulge. Fainter, bluer regions appear to extend outwards from the core, potentially indicating ongoing star formation, though on a relatively subdued scale. There's a hint of asymmetry in the outer regions, possibly indicative of minor gravitational interactions or tidal disturbances. The galaxy appears relatively isolated, with no obvious major companions visibly distorting its structure.
