The galaxy presents an overall smooth morphology, lacking any immediately obvious spiral arm structures or prominent dust lanes. It exhibits a somewhat elongated, elliptical shape, with an approximate axis ratio suggesting a moderate degree of flattening. The color gradient appears to transition from a bluish-white central region to a more reddish hue in the outer regions. This may indicate a concentration of younger, hotter stars in the core and older stellar populations in the periphery. There are no apparent signs of ongoing major merger activity or significant tidal disturbances, the galaxy appears relatively undisturbed.
