The galaxy presents as an elliptical morphology with a high degree of central concentration. The light profile appears smooth, lacking distinct spiral arm structures or prominent dust lanes. Color gradients suggest a population of older stars dominating the central regions, indicated by the yellowish hue. There is some evidence of bluer colors in the surrounding regions indicating recent star formation in small amounts. The galaxy exhibits a relatively high mass, with a corresponding low rate of star formation. The overall structure appears undisturbed, without signs of ongoing major merger activity. There is some evidence of minor disturbances that could be due to interactions or mergers. The general shape appears to be somewhere between round and cigar shaped.
