This galaxy appears to be an elliptical type, exhibiting a generally smooth, concentrated light profile. It's elongated in shape, appearing cigar-like from our viewing angle. A faint, diffuse structure is observed on the periphery, potentially indicative of tidal debris or a minor interaction with another galaxy. The dominant color is a yellowish-orange hue, suggesting a population of older stars. Star formation activity appears to be relatively low, based on the lack of discernible blue light associated with younger stellar populations. There are no distinct spiral arms or prominent dust lanes visible.
