The galaxy appears as a centrally concentrated system with a smooth, relatively featureless profile. There is a dominant, bright central bulge that suggests an older stellar population. Extending outwards from this central region is a faint disk. The light distribution within this disk is relatively even and doesn't show strong spiral arm structures or prominent star-forming regions. It has intermediate roundness, between round and cigar-shaped. There might be a hint of minor disturbance in the outer regions. The colors suggest a moderate amount of recent star formation, with the core being yellower, indicating older stars, with a bluer haze further out, indicating younger stars. Overall, the galaxy presents as an intermediate-mass system with moderate levels of on-going star formation activity.
