The object presents as a lenticular galaxy, viewed at an oblique angle. A central bulge is apparent, exhibiting a yellowish-white hue, indicative of an older stellar population. A disk surrounds the bulge, displaying a more bluish tint, suggesting the presence of younger, hotter stars and some ongoing star formation, though the rate appears to be low. The disk does not present tightly wound spiral arms, rather a more amorphous structure. There is some dust obscuration within the disk, creating a slightly mottled appearance. The galaxy exhibits an overall smooth appearance, with only minor disturbances. There is no indication of a major merger event, though minor tidal interactions cannot be ruled out.
