This galaxy exhibits a generally smooth morphology with a prominent central bulge. The light profile suggests a high degree of sphericity, though there is a slight elongation, presenting a shape somewhere in between round and cigar-shaped. The core appears quite luminous with a yellowish hue, indicative of an older stellar population. Fainter, bluer light is present in the outer regions, potentially suggesting some ongoing star formation, though it appears to be less significant than in the core. There is a very subtle hint of disk structure, but it is mostly dominated by the large smooth bulge. There is no clear evidence of any significant tidal disturbances or ongoing mergers. The galaxy appears to be relatively isolated and unperturbed.
