The galaxy presents as a relatively smooth, elliptical morphology. There is a high concentration of light in the central region, exhibiting a diffuse, bright core. The color profile suggests a redder core region, possibly indicating an older stellar population. Extending outward, the galaxy shows a transition to bluer hues in the outer regions, which may be indicative of younger star formation. The overall structure appears undisturbed, lacking any prominent spiral arms or significant signs of merging activity. The shape is noticeably elongated, with the ratio of the major to minor axes suggesting an elliptical type rather than a spherical one. The galaxy exhibits a gradual decrease in luminosity from the core to the outer regions, with a somewhat diffuse edge.
