The galaxy presents as an elliptical morphology, exhibiting a generally smooth and featureless appearance. The light distribution suggests a concentration toward the galactic center, with a gradual decrease in luminosity towards the outer edges. There is a slight elongation in the shape, approaching a cigar-like form. A subtle color gradient is visible, with the central region appearing more yellow, possibly indicating an older stellar population, while the outer regions show hints of bluer hues, suggestive of more recent star formation activity. No significant tidal disturbances or merging features are readily apparent.
