The galaxy presents as a centrally concentrated, luminous object. The light distribution appears relatively smooth, with a profile that suggests an elliptical morphology. The central region is bright and concentrated, gradually fading into the outer regions. The galaxy exhibits a yellow-red hue, indicative of an older stellar population with lower levels of ongoing star formation. There is no apparent disk structure, spiral arms, or significant dust lanes visible in the image. Overall, the galaxy appears to be a relatively undisturbed, mature system. The shape of the galaxy appears largely circular, though there is a slight deviation. There are no signs of strong tidal interactions or major mergers.
