The galaxy presents as an elongated, cigar-shaped structure with a smooth, diffuse appearance. The light distribution appears to be concentrated towards the center, which exhibits a warmer hue, transitioning to cooler tones towards the outer regions. The lack of readily apparent substructure suggests the absence of prominent spiral arms or distinct features. The galaxy's form is indicative of an elliptical morphology, although a highly inclined disk galaxy cannot be ruled out based solely on this imagery. There is no evidence of ongoing major mergers or significant tidal disturbances, though minor disturbances cannot be excluded. Overall, the galaxy appears relatively isolated and undisturbed.
