The galaxy presents as a fairly smooth, elliptical object with a concentrated central bulge. It appears nearly spherical, with minimal deviation from roundness. The color profile indicates a predominantly older stellar population, evidenced by its yellow-orange hue, suggesting a lack of significant ongoing star formation. There is no apparent evidence of spiral arms or a distinct disk structure. Additionally, there are no signs of major mergers or tidal disturbances. The galaxy appears to be an isolated, well-formed system in a relatively quiescent state.
