The galaxy appears to be an elliptical type, with a smooth, diffuse light distribution. The object exhibits a slightly elongated morphology, but lacks any distinct spiral arm structures or a prominent central bulge. The color suggests a population of older stars, exhibiting reddish hues characteristic of galaxies with low star formation rates. There is no evidence of significant dust lanes or active star formation regions, suggesting a relatively passive evolutionary state. There is no sign of any major disturbances or mergers.
