The galaxy appears to be an elliptical type, characterized by a smooth, diffuse light distribution. The morphology is elongated, exhibiting a cigar-shaped appearance, with a high degree of symmetry across its major axis. The central region is brighter and exhibits a yellowish hue, possibly indicative of an older stellar population. A gradual decrease in luminosity is observed from the core towards the outer edges of the galaxy. There is no discernible evidence of spiral arms or significant dust lanes. The overall structure suggests a relatively quiescent galaxy, with a likelihood of little current star formation. No obvious tidal features or distortions suggest a recent major merger event.
