The galaxy appears as a centrally concentrated object with a somewhat diffuse halo extending outwards. The core exhibits a bright, smooth profile, suggesting a prominent bulge component. The overall color is slightly bluish-white, which could indicate the presence of some younger, hotter stars and ongoing star formation, although not at a prodigious rate. The galaxy's morphology appears to be primarily elliptical. There is an indication of a possible minor disturbance or interaction, but not a major merger. The lack of clear spiral arms or a pronounced disk structure further supports a classification leaning towards an elliptical morphology with some transitional characteristics.
