The galaxy appears as a centrally concentrated, elliptical-like system. The light distribution is smooth, exhibiting a centrally-peaked bulge with a gradual decline in surface brightness moving outward. The color gradient is subtle; the central region seems to have a yellower hue compared to the fainter, outer regions which appear somewhat bluer. There is no evidence of distinct spiral arm structures or strong dust lanes. Overall the image appears to represent a spheroidal system with little ongoing star formation. There is no obvious visual evidence for any major ongoing merger activity. The morphology shows a lack of significant distortion, and no significant tidal features are detected.
