The galaxy presents an elongated, cigar-shaped morphology, indicating it is likely an elliptical galaxy. It exhibits a bright, centrally concentrated bulge with a noticeable radial gradient in surface brightness, fading towards the outer edges. There appears to be a disk component with a slight tilt relative to our line of sight. The galaxy exhibits a smooth, diffuse light distribution, with no apparent spiral arm structures. The color profile appears relatively uniform across the galaxy, with a slightly redder hue overall. No significant dust lanes or star-forming regions are readily apparent, suggestive of a relatively old stellar population and low star formation activity. There does not appear to be evidence of any major ongoing mergers or significant tidal disturbances.
