The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's structure, fading into a more diffuse halo. There's a subtle bluing in the outer regions of the disk, perhaps indicating some low-level star formation. There's no evidence of strong spiral arms or a well-defined disk, though a faint disk structure could exist. No major disturbances or merging events are immediately apparent, with only slight asymmetry that could potentially suggest minor tidal interactions or internal activity. Overall, the galaxy appears to be in a relatively relaxed state.
