The galaxy presents as a centrally concentrated system with a roughly circular morphology. The core region exhibits a yellowish hue, which may indicate an older stellar population. Surrounding the core, there is a more diffuse, greenish halo. This could be due to either a younger stellar population or ongoing star formation activity. The lack of any distinct spiral arm structure or prominent dust lanes suggests a relatively smooth distribution of stellar matter. There is no visually apparent evidence of tidal disturbances or interactions with other galaxies, suggesting it has undergone minimal recent merging events. It appears to be a relatively massive and luminous galaxy.
