The galaxy presents as a relatively smooth, elliptical-like structure, appearing somewhat elongated in shape. A bright, concentrated central bulge dominates the galaxy's core, gradually fading into a less defined, diffuse outer region. The color profile suggests a population of older stars, with a hint of bluer star formation in the outer regions. The galaxy does not display any prominent spiral arms or significant signs of ongoing major merger activity. There are suggestions of possible minor disturbances or asymmetries.
