The galaxy presents as an elongated, disk-like structure, with its major axis significantly exceeding its minor axis, suggesting a near edge-on orientation with respect to our line of sight. The central bulge exhibits a pronounced concentration of light, appearing smooth and spheroidal. Moving outward from the bulge, the disk gradually fades, displaying a subtle gradient in surface brightness. The disk component appears relatively smooth with no distinct spiral arm structure visible in the available imagery. The color profile indicates a bluer hue towards the outer regions of the disk, possibly indicative of ongoing star formation in those regions. No evidence of major mergers or significant tidal disturbances is apparent, though slight irregularities may be present in the disk morphology.
