The galaxy presents as an elliptical morphology with a generally smooth texture, displaying a concentrated central bulge that transitions into a fainter, more diffuse halo. The core region exhibits a yellowish-orange hue, suggesting a population of older, cooler stars. Moving outwards, the color shifts towards a slightly bluer tone, hinting at the presence of younger stellar populations, although not highly pronounced. No distinct spiral arm structures or prominent dust lanes are discernible, but the outer regions suggest a subtle disk-like structure. The galaxy does not appear to be significantly disturbed or undergoing a major merging event. The morphology is generally regular, with no apparent tidal tails or asymmetries, though there may be some minor disturbances visible in the outer disk. Overall, it appears to be a galaxy with intermediate to high mass, and with a relatively low star formation rate.
