The galaxy appears as a moderately bright, slightly elongated object. The central region exhibits a concentration of light, suggesting the presence of a galactic bulge or a central supermassive black hole. The overall color of the galaxy is a slightly yellowish-white, which suggests an intermediate stellar population. There is evidence of some bluer light in the outer regions, indicative of ongoing star formation. The galaxy appears relatively smooth in structure, with no readily apparent spiral arms or strong dust lanes, and the overall morphology is somewhat disk-like in appearance. There is a subtle indication of a minor disturbance, perhaps a very weak tidal feature or interaction, with a slight asymmetry in the distribution of the galaxy's light. The galaxy's size, based on the data, indicates that it is a relatively large galaxy with significant mass.
