The galaxy appears as a single, somewhat diffuse object with a concentrated core region. It is roughly elliptical, exhibiting a slight elongation but appearing generally rounded. The color profile suggests a mature stellar population, leaning towards redder hues. There is little evidence of spiral arm structure or significant dust lanes. Overall, the galaxy presents a smooth and featureless morphology, suggesting a classification as an elliptical galaxy. Subtle irregularities in the outer regions hint at possible past minor interactions.
