The galaxy presents a predominantly smooth morphology. Its shape appears generally rounded, exhibiting a slight ellipticity rather than a distinctly elongated or cigar-like form. The color profile suggests a dominant population of older stars, yet there's evidence of ongoing star formation, concentrated towards the center, indicated by a faint bluish-green hue. No major disturbances or signs of an ongoing merger event are immediately apparent, though subtle asymmetries might suggest minor past interactions. The galaxy exhibits a notable central concentration of light, with a gradual decrease in luminosity towards its outer regions.
