The galaxy presents as a centrally concentrated, generally smooth structure. It exhibits an elliptical morphology, appearing largely spheroidal, with a slight elongation noticeable. The central region of the galaxy is significantly brighter and displays a yellowish hue, indicating a population of older stars. Moving outwards from the center, the light gradually diminishes and transitions to a bluer tint, suggesting the presence of a younger stellar population in the galaxy's outskirts. There is no clear evidence of spiral arm structures or significant dust lanes within the galaxy's visible morphology, implying a relative lack of ongoing active star formation compared to its past. Slight disturbances are observed in the outer regions but are minor. Overall, the galaxy appears to be a relatively massive early-type galaxy with a dominant spheroidal component.
