The galaxy appears as a single, relatively bright object. Its overall structure is smooth, exhibiting a somewhat elliptical morphology, with a slightly elongated shape. The color profile suggests a dominant population of older stars, with an orange-yellow hue. There is no visible evidence of significant spiral arm structure or dust lanes, indicating it is likely an early-type galaxy, potentially an elliptical or lenticular type. There are no clear signs of a recent major merger event, although some faint irregularities in the outer regions may suggest minor tidal interactions or past accretion events. Based on its color, and smooth appearance, this galaxy appears to have a low star formation rate. The galaxy is relatively compact in size.
