The galaxy presents as a somewhat elongated, yet mostly smooth, elliptical morphology. It displays a bright central bulge, with the luminosity appearing to gradually decrease towards the outer edges. There is little indication of spiral arm structures or prominent dust lanes. The color profile suggests a population of older stars with a general lack of prominent star forming regions, likely due to the redder appearance. Subtle color variations towards the outer edges might indicate areas of differing stellar populations or residual star formation. The shape is somewhere between round and a cigar shape. Overall, it looks like a fairly relaxed system, potentially having undergone past minor disturbances.
