The galaxy presents as an elliptical or lenticular morphology, exhibiting a generally smooth and concentrated light distribution. There is a relatively high degree of central concentration. The galaxy appears somewhat elongated, but not highly so, with an intermediate axis ratio. No distinct spiral arms or prominent features such as bars are readily apparent in the image.

The color profile shows a yellowish central region, possibly indicative of an older stellar population and/or a higher concentration of dust. The outer regions exhibit a subtle blueish tint in comparison, potentially signaling the presence of some younger, hotter stars, though it could also just be a result of a decreasing presence of dust. There is no visual evidence of a recent major merger or significant tidal disturbance. The overall impression is that of a relatively evolved system.
