The galaxy presents as a roughly elliptical, albeit somewhat disturbed, morphology. There appears to be a smooth central bulge exhibiting a yellowish-orange hue, suggesting a population of older stars. Moving outward, a fainter, bluer disk-like structure is visible, indicating ongoing or recent star formation. There's a slight asymmetry in the outer regions, potentially indicative of a minor interaction or tidal disturbance. Based on the relatively compact size and overall appearance, this galaxy appears to be an intermediate-mass system undergoing a transition in its star formation activity, from quiescent in the bulge to active in the outer regions.
