The galaxy presents as a relatively small, elongated structure. The morphology appears to be that of a flattened ellipsoid, exhibiting a cigar-like shape. The luminosity distribution across the galaxy seems to be relatively smooth, with a slight central concentration but without a pronounced bulge. There is some evidence of a faint disk-like structure, but it is not well-defined. Color gradients within the galaxy are subtle, suggesting a relatively homogenous stellar population. There is no apparent evidence of any major mergers or tidal disturbances. The object appears to be relatively isolated.
