The galaxy presents an elongated, cigar-shaped morphology, strongly suggestive of an elliptical galaxy viewed nearly edge-on. The primary color is a yellow-orange hue, indicating a stellar population dominated by older, cooler stars. There is little to no visual evidence of spiral arm structure or significant dust lanes. The light distribution is relatively smooth and concentrated, with a gradual fading towards the outer edges of the galaxy. This suggests a lack of ongoing, large-scale star formation within the galaxy's visible structure. The shape and color profile is consistent with a high mass and a relatively low specific star formation rate. There is no visually apparent sign of recent mergers or major tidal disturbances.
