The galaxy presents an elliptical morphology, exhibiting a generally smooth light distribution with minimal discernible substructure. There is a slight elongation, giving it a shape that falls between perfectly round and cigar-shaped, more along the lines of a slightly squashed circle. The galaxy exhibits a color gradient, with the central region appearing more reddish, and the outer regions appearing more bluish, hinting at either a decreasing metallicity gradient or a potential recent merger event that is not clearly seen. The galaxy does not appear to be undergoing any major mergers or showing signs of significant tidal disturbances, indicating that it is likely in a relatively quiescent state. Its compact appearance and smooth profile are consistent with an evolved stellar population, possibly dominated by older stars.
