The galaxy presents as a smooth, elongated structure. Its overall shape appears to be somewhere between round and cigar-shaped, appearing somewhat flattened, likely an elliptical morphology seen at an angle. The galaxy exhibits a color gradient, transitioning from a bluer hue at the outer edges to a more concentrated, brighter, and slightly yellower central region. This suggests a higher concentration of older stars and a lower rate of star formation within the core compared to the outer regions where younger, bluer stars may be present. The light distribution is fairly uniform, indicating that it is most likely not undergoing any major merging events or major disturbances. Subtle, irregular features or minor disturbances cannot be ruled out entirely, but its appearance is consistent with a relatively quiescent galaxy.
