The observed galaxy presents as a relatively compact object with a noticeable central bulge. While appearing somewhat smooth, the image suggests the presence of subtle features indicative of a possible disk structure. There appears to be a slightly irregular shape possibly due to a minor gravitational interaction. A faint halo of light surrounds the galaxy, gradually fading into the background sky. The color distribution indicates that the central region may host an older stellar population, while the outer regions show hints of bluer colors, suggesting ongoing or recent star formation. Overall, the galaxy appears to be in a relatively undisturbed state, yet possesses subtle characteristics suggesting it is not entirely featureless.
