The galaxy presents as a relatively compact object with a smooth, centrally concentrated light distribution, indicative of an elliptical or lenticular morphology. There appears to be a slight elongation, although the overall form is largely rounded. The galaxy exhibits a color gradient, with a reddish hue dominating the outer regions and transitioning to a bluer, potentially younger stellar population towards the core. The absence of obvious spiral arm structures or dust lanes further supports the classification of a passively evolving system. There is no strong evidence of any tidal features or ongoing major mergers. The red shift indicates the galaxy is a significant distance away.
