The galaxy presents as a somewhat elliptical, diffuse structure. A central bulge is apparent, exhibiting a yellowish hue that likely indicates an older stellar population. The surrounding disc appears less defined, displaying a mottled blue-ish color, potentially indicative of ongoing star formation. There is some evidence of minor disturbances in the overall morphology; one portion of the disk appears more luminous, suggesting possible interactions or tidal effects. The lack of clear spiral arm structure suggests that this galaxy is most likely an intermediate type.
