The galaxy appears as a centrally concentrated object with a smooth, somewhat elliptical morphology. A bright, unresolved core suggests the presence of a significant stellar bulge or a possible active galactic nucleus, though no clear jet is visible. The surrounding diffuse light indicates a larger, less dense halo component. There is minimal evidence of spiral arm structure or distinct star-forming regions within the visible extent of the galaxy. Its color is generally yellowish, hinting at an older stellar population. No signs of major interactions or mergers are immediately apparent, although subtle asymmetries might indicate a previous minor disturbance or ongoing accretion event.
