The galaxy presents as a slightly elongated, disk-like structure seen at an oblique angle. There is a noticeable color gradient, with a bluer hue concentrated in what appears to be a central bulge, and a shift towards redder tones in the outer regions. This color difference suggests a distribution of stellar populations, with younger, hotter stars residing in the central region, indicative of possible recent or ongoing star formation. The overall smoothness of the light distribution suggests that the galaxy lacks prominent spiral arms or other strong features. A fainter, diffuse halo may be present, extending slightly beyond the brighter central region. The appearance is suggestive of an elliptical galaxy with some disk-like features, or potentially a spiral galaxy with tightly wound arms and a dominant central bulge. Some tidal disturbance appears to be present.
