The galaxy presents an elliptical morphology with a smooth, concentrated central bulge that transitions into a fainter, more diffuse halo. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. The disk component is less pronounced, appearing as a faint, flattened structure surrounding the bulge. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers, although there seems to be a minor irregularity in the disk's shape. The disk component exhibits a bluer tint compared to the bulge. Overall, the galaxy shows characteristics of a relatively massive system with a low ongoing star formation rate.
