The galaxy presents a flattened, elongated morphology, appearing cigar-shaped in its overall structure. There is evidence of a relatively smooth light distribution, with a central concentration of luminosity suggesting a bulge. Hints of a disk-like structure are visible, though it is not prominently defined. The galaxy exhibits a blueish hue in its outer regions, potentially indicating regions of star formation. However, the overall color gradient suggests that the stellar population is primarily older, with a transition towards redder colors within the central bulge, which may indicate a population of older stars, less active star formation. There are no obvious signs of ongoing major mergers or significant tidal disturbances.