The galaxy presents as a relatively small, faint, and moderately distant object. It appears largely smooth and elliptical in morphology, with a central, bright bulge that dominates the overall light profile. There is a subtle, but discernible disk feature. There appears to be some degree of minor disturbance or irregularity in the outer regions, possibly suggestive of a past or ongoing interaction. The object exhibits a moderate color gradient, with the central region appearing slightly redder, possibly indicating an older stellar population, while the outer regions exhibit bluer hues, potentially signifying younger stars or ongoing star formation, though the latter appears to be at a low rate. The galaxy's estimated mass indicates it is a dwarf galaxy.
