The galaxy appears as a single, unresolved, centrally concentrated object with a smooth morphology. Its color is predominantly yellowish-orange, suggesting an older stellar population. The lack of visible spiral arms or distinct features indicates a likely spheroidal or elliptical shape. There is no apparent evidence of recent or ongoing major merging activity. A slight elongation is present, suggesting that the galaxy is not perfectly circular. The galaxy's high degree of smoothness suggests that it is a relatively evolved system. The light is dominated by redder wavelengths, indicating little ongoing star formation.
