The galaxy presents as a somewhat elliptical or lenticular structure with a smooth overall appearance. The central region exhibits a yellowish-white hue, indicative of an older stellar population. Patchy regions of redder color are observed, possibly indicating areas of dust obscuration or ongoing star formation. The galaxy does not show clear spiral arm structure or a prominent central bulge, but a slight disk feature is visible. There may be minor disturbances visible in the disk structure, but this may also be a result of artifacts. The galaxy appears to be relatively isolated, with no apparent signs of major mergers.
