The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. A subtle disk component appears to exist as the outer regions of the galaxy fade gradually into the background. The galaxy appears to be primarily yellowish-white, suggesting an older stellar population. There is little indication of ongoing, significant star formation activity, as evidenced by the lack of distinctly blue regions or prominent spiral arms. The overall structure suggests that it is in a relatively relaxed state, with no major signs of recent mergers or significant tidal disturbances. A slight asymmetry is noticeable in the outer regions, possibly indicating minor past interactions, or internal processes. The rounded, somewhat featureless morphology reinforces the classification as a galaxy with a dominant spheroidal component.
