The galaxy presents as an elliptical or lenticular type. It exhibits a generally smooth morphology with a concentrated central bulge region. This central area is bright, indicating a high density of stars. Moving outward from the center, the light gradually diffuses, suggesting a decrease in stellar density. The galaxy has a slightly elongated shape, deviating from a perfect sphere. No distinct spiral arm structures or prominent dust lanes are discernible in this image. There is a subtle color gradient apparent, with the central region appearing slightly bluer and the outer regions exhibiting a reddish hue. This may indicate older stellar populations in the outskirts. Minor disturbances are potentially present, perhaps due to minor interactions.
