This galaxy presents as a relatively smooth and rounded structure. It exhibits a concentrated central bulge that transitions smoothly into a fainter, more diffuse halo. There is a subtle color gradient, where the central region appears somewhat bluer compared to the outer edges, which possess a slightly redder hue. No distinct spiral arms or bar-like features are immediately apparent, giving the galaxy a lenticular or possibly elliptical appearance. There are no signs of significant tidal disturbances or ongoing major mergers. The lack of prominent dust lanes suggests a relatively low gas and dust content. The galaxy appears to be relatively isolated, without close companions or signs of strong gravitational interactions.
