The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards. The dominant color is a warm yellow-orange hue, suggestive of an older stellar population. There's a slight asymmetry, possibly indicative of a minor interaction or internal structure. No distinct spiral arms or prominent dust lanes are discernible. Overall, the galaxy presents a fairly regular and well-defined morphology.
