The galaxy presents as a relatively smooth, elliptical object with a prominent bulge. The central region exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer regions are subtly present in what may be the outer disk or extended halo, indicating the possibility of some ongoing star formation. The galaxy appears somewhat elongated, exhibiting a cigar shape. There are no obvious signs of major mergers or tidal disturbances. Based on its apparent morphology and color profile, this galaxy is likely a massive, evolved system, exhibiting a low specific star formation rate.
