The galaxy presents a relatively smooth morphology, displaying characteristics of an early-type system. It exhibits an elliptical shape, with an aspect ratio suggesting a classification between E4 and E6. The light profile is centrally concentrated with a bright core, and it fades gradually toward the outer regions. Little to no discernible spiral arm structure is visible. There is a subtle color gradient, with the core appearing more yellow, possibly indicating an older stellar population, while the outer regions show a slightly bluer hue. This hints at a small amount of ongoing or recent star formation, particularly in the outskirts. No significant dust lanes or prominent tidal features are observed, which would suggest recent major merger events. The overall appearance suggests a galaxy in a relatively quiescent state, with a dominant population of older stars and limited current star-forming activity. Any ongoing star formation is likely occurring at a low rate.
