The galaxy presents a smooth, elliptical morphology. Its shape appears elongated, approaching a cigar-like structure. The light distribution is concentrated towards the center, exhibiting a relatively bright core that fades gradually towards the outer edges. There is no apparent presence of spiral arms or prominent dust lanes, which suggests that the galaxy may be an elliptical type. Signs of mergers or tidal disturbances are very weak, indicating that the galaxy has remained relatively undisturbed. The color profile suggests a population of older stars dominating the light, giving the galaxy an overall yellow/red hue. There is no evidence of bright, young stars dominating the light, indicating low current star formation. The galaxy is compact in size.
