The galaxy presents an elongated, cigar-shaped morphology, suggesting it is likely an elliptical or lenticular galaxy viewed at an angle. The central region exhibits a concentrated brightness, appearing smooth and relatively featureless. Proceeding outward, the intensity gradually decreases. There is a color gradient visible; the central core is a yellowish/reddish hue while the outer regions possess a greenish tint. The redder color may indicate an older stellar population dominating the core, while the green is likely from Hydrogen emission lines due to areas of star formation.
