The galaxy presents a generally smooth and rounded morphology. There is a slight elongation or cigar shape apparent in the visual structure. The central region is notably brighter and exhibits a reddish hue, potentially indicative of an older stellar population. The outer regions appear less concentrated and display a bluer color, possibly associated with younger stars or ongoing star formation. There is no strong evidence of major disturbances or ongoing mergers, although there are minor irregularities that could indicate minor interactions. The color gradients suggest a radial distribution of stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars in the outer regions. Overall, the galaxy appears to be a relatively evolved system with a mix of stellar populations.
