The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, luminous core with a yellowish hue, suggesting an older stellar population dominating this area. Moving outward from the core, the galaxy shows a gradual decrease in luminosity. A subtle blueish tint is observed in the outer regions, which could indicate the presence of younger, hotter stars, potentially associated with ongoing or recent star formation activity, albeit at a relatively low level. The overall shape is more of a disc than a perfect spheroid, and there are no signs of strong tidal disturbances or ongoing major mergers, but there seems to be some minor disturbance or other interaction.
