The galaxy presents a generally smooth, elliptical morphology, with the light profile appearing more concentrated towards the center. The dominant color is a yellow-orange hue, suggesting a population of older stars. There appears to be a slight elongation in the galaxy's shape, hinting at a possible transition between elliptical and lenticular morphology, though no distinct disk-like structure is clearly visible. There is no visible spiral structure or strong evidence of recent major mergers or tidal disturbances. Faint, diffuse extensions of the galaxy's halo may be present, though they are difficult to discern definitively from the background. The galaxy is a relatively luminous object at its estimated distance, suggesting a high stellar mass. There may be some low levels of ongoing star formation, but the overall stellar population appears to be aging. 
