The galaxy presents as a generally smooth and elliptical object, approximately 6.2 kpc in effective radius. It appears to be largely spheroidal in shape but may be slightly cigar-shaped. The central region exhibits a distinct yellowish-orange hue, potentially indicative of an older stellar population. A faint, diffuse halo of bluish light surrounds the central bulge, perhaps signifying a small amount of ongoing star formation. There are no apparent spiral arms or other distinct features, and no major signs of any merging activity, although there appears to be minor disturbances in the outskirts. The galaxy does not appear to be particularly dusty, as there is no significant reddening.
