The galaxy presents as a single, somewhat diffuse object exhibiting a slightly elongated morphology. It's light profile appears fairly smooth, showing a general concentration toward a bright central region, which is possibly the galactic nucleus. There are hints of features that might represent the merging of another smaller galaxy or the after effects of a collision. The distribution of light indicates that the galaxy might be disk-shaped or elliptical. It appears to be quite compact. The color profile is dominated by yellowish hues, suggesting a population of older stars and relatively low current star formation.
