The galaxy presents a predominantly smooth morphology. The light is centrally concentrated and elliptical in shape, with the majority of light emitting from the central region. A faint disk structure is barely visible beyond the central bulge. The core is golden in color, slowly transitioning into cooler blues at the edge of the galaxy. There appears to be a small bulge to the left of the main core. There is very little evidence of spiral arms. The galaxy exhibits some minor disturbances in its overall structure. These could suggest past interactions or minor merger events that have disrupted its initial formation. The colors suggest that there is some ongoing star formation, but is dominated by an older stellar population.
