The galaxy exhibits a generally elliptical morphology. The central region presents a bright, concentrated core with a cyan hue, possibly indicating strong emission lines or a higher concentration of younger, hotter stars. This central concentration is slightly elongated along the major axis of the galaxy.

Extending outward from the core is a fainter, more diffuse disk. This disk appears relatively smooth with some faint hints of structure. The outer regions of the disk fade gradually into the background, showing no sharply defined edges. The galaxy's overall color gradient shifts from cyan in the core to a slightly redder tone in the outer regions, consistent with an aging stellar population in the outskirts. 

There is an apparent disturbance in the overall structure, which might be indicative of a potential minor merger or tidal interaction.
