This galaxy exhibits a generally smooth morphology, appearing as an elliptical structure with a central concentration of light. It has a moderately elongated shape and is an orange hue, suggestive of an older stellar population. There is evidence of a possible minor interaction or merger event, as indicated by a smaller, nearby component. This component appears as a slightly fainter, rounder object in close proximity to the main galaxy body. While the majority of the galaxy's light is centrally concentrated, there is a slight extension to the overall light distribution. There is no evidence of spiral arms, or a prominent disk. Overall, the galaxy appears to be a relatively evolved system, possibly a lenticular or early-type elliptical undergoing a minor interaction.
