This galaxy exhibits an elliptical morphology, with a smooth, concentrated luminosity profile. The overall shape is moderately elongated, appearing somewhere between a perfectly round and a cigar-like form. There is no obvious spiral structure or distinct disk component visible. The galaxy's core is a bright, concentrated yellowish-white, suggesting an older stellar population dominates the central regions. The surrounding halo exhibits a gradual decrease in luminosity with increasing radial distance from the center and is more reddish compared to the core, consistent with an aging stellar population and potentially higher dust content. There is no evidence of ongoing major mergers, though subtle asymmetries in the outer regions might suggest minor gravitational interactions in its past. The overall color indices imply moderate levels of recent or ongoing star formation, although not as significant compared to bluer spiral galaxies. 
