The galaxy exhibits a generally smooth, elliptical morphology. There is a concentrated, bright central bulge which fades into the outer regions. The color profile suggests a relatively old stellar population, with a redder hue in the central region indicative of older stars. The outer regions exhibit a slightly bluer color, suggesting the presence of a younger stellar population, though not drastically so. There is no clear evidence of spiral arms or a significant disk structure; the light appears to be more uniformly distributed. The overall appearance suggests a relatively relaxed, evolved system. There is some minor evidence of a slight disturbance in the galaxy's shape, although its appearance is overwhelmingly relaxed and regular. 
