The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arm structures or distinct features associated with active star formation. The galaxy exhibits a yellow-orange hue, suggesting a population of older stars. The absence of prominent dust lanes or blue-shifted regions indicates that the star formation rate within the galaxy is subdued. There is some minor disturbance in the shape, potentially due to a past minor merger event. The galaxy exhibits a relatively round shape and is not highly elongated. Overall, this galaxy appears to be a relatively evolved system that is not currently undergoing significant star formation.
