The galaxy presents as a central, moderately bright, and somewhat diffuse object with a slightly elongated morphology. The core region appears primarily smooth and concentrated, exhibiting a yellowish-white hue, which suggests a population of older stars dominating the light output. The galaxy lacks any readily discernible spiral arm structure. Fainter, bluer light extends outward from the central region, indicating the presence of some younger stars or ongoing star formation, but it is not particularly prominent. Overall, the galaxy's light profile is smooth and relatively uniform. There is no evidence of a major ongoing merger or significant tidal disturbances.
