The galaxy presents a largely smooth and somewhat elliptical morphology. Its central region appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue, indicative of a lack of recent star formation in the core. The outer regions show a fainter, bluer tint, suggesting the presence of younger stars or ongoing star formation, albeit at a lower rate compared to more active spiral galaxies. There's a slight asymmetry in the outer isophotes, but no clear evidence of major disturbances or ongoing mergers are immediately apparent. The galaxy appears to be relatively isolated within the observed field.
