The galaxy presents as a centrally concentrated object with an overall smooth morphology. There is a distinct core region exhibiting a yellowish-white hue that suggests a population of older stars. The galaxy appears largely spheroidal in shape, and the light fades gradually from the center outward, showing no clear spiral arm structures or distinct features. There is a slight elongation visible. There are faint, irregular structures surrounding the core region, potentially dust or tidal debris, suggesting a possible history of minor interactions. The galaxy exhibits a relatively low rate of star formation based on color.
