The galaxy presents a primarily smooth morphology, with a suggestion of disk-like features. The central bulge exhibits a bright, concentrated luminosity, transitioning into a less defined, extended halo. The overall shape is neither perfectly round nor elongated, leaning more towards an intermediate form. There is a subtle hint of potential gravitational disturbance, possibly indicating a minor interaction. Overall, the galaxy displays intermediate star formation activity. The estimated size places it in the range of a typical galaxy. Color index shows a slight increase in redder bands, possibly indicating older stellar populations within the bulge.
