The galaxy presents as an elliptical morphology, elongated with a cigar-shaped appearance. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, possibly indicating an older stellar population. The outer regions gradually fade into a reddish halo, suggesting a more diffuse distribution of stars. The light distribution appears smooth with no distinct spiral arm structures or prominent dust lanes visible. There is a suggestion of ellipticity, where the galaxy is more than twice as long as it is wide. No significant signs of tidal interactions or ongoing major mergers are immediately apparent.
