This galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a largely featureless morphology. It presents as a centrally concentrated luminosity profile, with a gradual decrease in brightness outwards from the core. The galaxy appears approximately round in shape. There is a slight color gradient, transitioning from a predominantly yellow-orange core to a greenish-blue hue in the outer regions. This color variation suggests that the central region may host an older stellar population, while the outer regions potentially contain a younger, bluer population of stars or ongoing star formation, though at a low rate. There is no visually significant evidence of spiral arms, bars, or ongoing major mergers, although minor disturbances are not entirely ruled out. Overall, the galaxy seems to be relatively isolated and undisturbed.
