The galaxy presents as a roughly elliptical structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy show a bluer tint, possibly indicating the presence of younger stars and ongoing star formation, although not with high intensity. There are hints of disturbances within the galaxy's structure, potentially the result of a minor interaction or internal processes. The galaxy exhibits characteristics of an intermediate disk galaxy with a dominant bulge. The morphological classification leans toward the 'smooth or featured' category, with a moderately rounded appearance. No strong tidal tails or other major merger features are obviously present.
