The galaxy presents a generally smooth, elliptical morphology with a high degree of roundness. There is little evidence of significant disk structure or spiral arms. The central region exhibits a bright, concentrated luminosity profile, suggesting a prominent bulge. The color profile indicates a slightly redder core, potentially indicative of an older stellar population. The outer regions appear marginally bluer, perhaps due to recent or ongoing star formation, although the overall star formation rate is relatively low. No major merging activity or tidal disturbances are readily apparent, although some minor asymmetry could suggest past interactions or internal processes. The estimated size of the galaxy is moderately large.
