The galaxy presents as a relatively smooth, elliptical structure. It is elongated, exhibiting a cigar-like shape. The central region displays a concentrated luminosity, suggesting a significant stellar population and/or an active galactic nucleus. Moving outward from the core, the light gradually diffuses, indicating a decreasing stellar density. There appears to be a subtle color gradient, transitioning from slightly yellow at the core to a slightly bluer hue in the outer regions, which may reflect differences in stellar populations and ages. No prominent spiral arms or distinct features are visible; therefore, a classification as an elliptical galaxy is appropriate. There are no apparent signs of tidal disturbances or ongoing mergers, and the overall morphology suggests a relaxed and relatively quiescent state.
