The galaxy presents a predominantly smooth morphology. It appears elliptical in shape, with a high degree of central concentration. The color profile suggests a population of older stars, contributing to its reddish-gold hue. There's little evidence of spiral arms or significant dust lanes. A slight asymmetry in the outer regions hints at a possible minor interaction or disturbance, but the overall structure appears relatively undisturbed. The lack of prominent blue regions indicates a low rate of ongoing star formation. The estimated size of the galaxy appears moderate, suggesting an intermediate mass range.
