The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears fairly uniform, with a noticeable color gradient from a more yellowish-white core to a slightly redder outer region. There is no apparent spiral arm structure or dust lane obscuration. The galaxy appears relatively isolated, without obvious signs of tidal interactions or a recent merger event. The round morphology suggests a lack of significant rotational support, consistent with an early-type classification. The color indicates that it may be a lenticular galaxy. Overall, the galaxy appears to be a mature system with a dominant population of older stars.
