The galaxy presents as a centrally concentrated, luminous object with a generally smooth appearance. The primary body exhibits a yellow-white hue, suggesting a population of older stars. There is a noticeable lack of defined spiral arms or a prominent disk structure, supporting a classification leaning toward an elliptical or lenticular morphology. A small, fainter, and bluer patch is seen adjacent to the main body, possibly indicating a region of recent star formation or a smaller companion galaxy experiencing tidal disruption. Overall, the galaxy appears relatively isolated with no obvious signs of ongoing major merger activity. The overall shape appears moderately elliptical, not perfectly round but not extremely elongated. There is a potential minor disturbance or faint tidal feature extending from the galaxy, but the data suggest a mostly relaxed state.
