The galaxy presents a generally smooth morphology, although subtle irregularities can be observed upon closer inspection. Its shape is somewhat elongated, leaning toward a cigar-like form, though a dominant central bulge suggests characteristics between elliptical and lenticular classifications. The galaxy exhibits a color gradient, appearing bluer at the periphery, indicating the presence of younger stellar populations, and redder towards the core, which is consistent with older, more evolved stars. There appears to be no significant evidence of ongoing major mergers, or significant tidal distortions. However, I cannot rule out minor interactions given the spatial resolution of the image. 
