The galaxy presents as a centrally concentrated object with a generally smooth morphology. The overall shape approximates a flattened ellipsoid, appearing nearly round. There is a distinct central bulge exhibiting a yellowish hue, suggesting an older stellar population is dominant in this region. Fainter and bluer emissions extend outwards from the central bulge, indicative of regions with ongoing star formation. There is no obvious presence of a grand design spiral structure or a prominent bar. The galaxy displays a slight asymmetry in its outer regions. The lack of significant tidal features or nearby companions suggests it is likely not undergoing a major merger. The overall appearance points toward a galaxy undergoing a transition from active star formation to a more quiescent state.
