The galaxy presents as a smooth, elliptical-like structure with a notable central bulge. The light distribution appears more concentrated towards the core, diminishing gradually towards the edges. The galaxy exhibits a slight elongation, suggesting a shape that is somewhat cigar-like. The colour profile indicates an older stellar population dominating the central region, identified by the reddish hue, while bluer tones are observed in the outer regions, possibly indicating some ongoing star formation, albeit at a modest rate. There are no readily apparent signs of significant tidal disturbances or interaction with other galaxies. The galaxy appears relatively isolated and undisturbed.
