The galaxy presents as an elliptical morphology with a smooth, largely featureless appearance. Its light is concentrated toward the center, exhibiting a bright central bulge that fades gradually into the outer regions. The galaxy appears moderately flattened, with a slight elongation visible along one axis. There is no clear evidence of spiral arms, dust lanes, or ongoing major mergers. Overall, the galaxy seems to be a relatively undisturbed system. The color profile suggests an older stellar population, with light tending toward the redder end of the spectrum, specifically a yellow hue.
