The galaxy presents as a single, relatively smooth object with a concentrated central bulge. Its overall shape is elliptical, exhibiting a generally round morphology. The color profile is dominated by reddish hues in the core, transitioning to greenish tones in the outer regions. There appears to be some minor irregular structure at the periphery, perhaps indicating a weak interaction or recent accretion event. The light distribution suggests a galaxy dominated by an older stellar population, potentially with ongoing low-level star formation. There is no evidence of a prominent disk structure or spiral arms.
