The galaxy presents as a largely featureless, elliptical-like structure. Its color profile is centrally concentrated with a yellowish hue at the core transitioning to a bluer, fainter periphery. There is a slight elongation, but overall the shape appears close to round. There is no evidence of spiral arms or a distinct disk component. Subtle irregularities in the outer regions may indicate minor disturbances, but the dominant impression is that of a relaxed system. Based on the color indices, the stellar population may be moderately old. Star formation is still likely occurring, though at a relatively low rate, as evidenced by the blue outer regions. The object does not appear to be undergoing a major merger or significant tidal interaction.
