The galaxy presents as a relatively compact object. It exhibits a generally smooth, elliptical morphology, with a high degree of central concentration. The light profile suggests a lack of spiral arm structure or significant disk features. The color appears slightly redder towards the core, potentially indicating an older stellar population or increased dust obscuration in that region. There's a subtle elongation in shape, neither perfectly round nor strongly cigar-shaped. Faint asymmetrical features are visible but do not suggest a major ongoing merger event; they might be indicative of a minor interaction or tidal disturbance in the past. Overall, the galaxy is a relatively quiescent system.
