The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears yellowish in color, possibly indicating an older stellar population. The galaxy's overall shape is moderately elongated; appearing somewhat cigar-shaped. There is little evidence of strong spiral arm structures or significant dust lanes, although subtle color variations suggest some internal structure or ongoing, but limited, star formation. No major merger events are immediately apparent, though subtle asymmetry is visible. The outskirts fade gradually into the background, hinting at an extended halo of stars.
