The galaxy presents a generally smooth, elliptical morphology. Its overall shape is largely rounded, with a slight suggestion of elongation that doesn't fully classify it as cigar-shaped. A dominant central bulge is present, exhibiting a concentrated and bright luminosity, suggesting a high density of stars. The galaxy color profile indicates a redder hue within the core region, transitioning gradually to a bluer tone towards the outer regions. This implies an aging stellar population with suppressed star formation rate. No obvious spiral arms, bar structures, or merging signatures are observed, and no significant tidal disturbances are observed within the galaxy's structure.
