The galaxy appears to be a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is fairly uniform, fading gradually from the center outwards, exhibiting a round shape. The galaxy presents with a yellowish-orange color, potentially indicating an older stellar population and a lack of significant ongoing star formation. No distinct spiral arms or dust lanes are visible. There is no indication of any major tidal disturbances or ongoing mergers. The morphological features suggest that this is most likely a galaxy that is largely composed of older stars.
