The galaxy presents as a somewhat elliptical, relatively smooth structure, with minimal visible features such as spiral arms or dust lanes. The galaxy exhibits a color gradient, appearing more yellow-white towards the center and transitioning to slightly bluer hues at the edges. This suggests a possible variation in stellar populations, with older, redder stars concentrated towards the core and younger, bluer stars more prevalent in the outer regions, although the color difference is slight. The galaxy shows a high degree of central concentration. There is no indication of a significant merger event or tidal disturbance. The overall shape is not perfectly round; the galaxy seems slightly elongated. The light distribution indicates that this is not a late-type spiral galaxy, and appears more like an elliptical galaxy with an estimated size of 4.3 kiloparsecs. There is little evidence of ongoing star formation.
