The galaxy appears as a somewhat elongated structure, exhibiting a central bulge region that is brighter and has a yellowish hue. This suggests a population of older, redder stars concentrated towards the galaxy's center. Extending outwards from the central bulge, we observe fainter, bluer regions. These regions likely contain younger, hotter stars and may indicate ongoing star formation.

The galaxy seems to have a somewhat disturbed morphology, as evidenced by slight irregularities in its shape and subtle asymmetric features in the outer regions. The overall color gradient suggests a transition from older stellar populations in the center to younger populations in the outer regions. The size of the galaxy is relatively compact, and it doesn’t show any obvious signs of strong tidal interactions.
