The galaxy presents as a single, relatively smooth object with a centrally concentrated light profile. There is no distinct spiral arm structure visible in this image, nor is there evidence of a prominent bar. The galaxy appears nearly circular, with a high degree of central symmetry, suggesting a classification leaning towards elliptical or lenticular.

The color gradient indicates a slightly bluer center, transitioning to redder hues in the outer regions. This could point to older stellar populations dominating the outskirts, with a possible central region of ongoing or more recent star formation. The overall light distribution is relatively even, lacking pronounced knots or irregularities that would suggest a recent or ongoing major merger event. Minor disturbances may be present, but the overall morphology is largely undisturbed. The estimated size indicates this is a moderately sized galaxy. Overall, it looks like a large, relatively undisturbed galaxy, exhibiting an aged stellar population.
