The galaxy presents a generally smooth morphology, suggesting a lack of prominent spiral arms or distinct features usually associated with actively star-forming galaxies. Its overall shape is somewhat elliptical, appearing more "in between" elliptical and round than distinctly flattened or cigar-shaped. A concentration of light is observed toward the center, indicating a central bulge. The galaxy exhibits a color gradient, with a yellowish-white hue dominating the central regions, possibly indicative of an older stellar population. There is a suggestion of bluer light in the outer regions, which may be due to the presence of a younger stellar population. There is no clear evidence of any major mergers or tidal disturbances in the immediate vicinity of the galaxy.
