The galaxy presents as a moderately bright, elliptical or lenticular system, exhibiting a relatively smooth morphology. The central bulge region appears prominent, displaying a concentrated intensity of light. There is some indication of a disk-like structure, but the overall light distribution suggests the galaxy is primarily bulge-dominated. The color profile indicates a population of older stars, with a yellowish-orange hue predominating. There are some traces of blue in the outer edges, which potentially indicates the presence of younger stars, but the star formation rate is overall low. There is some evidence of minor tidal disturbances to the galaxy, although it does not seem to be undergoing a major merger event. The galaxy seems to be relatively isolated.
