The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology. It lacks prominent spiral arms or a well-defined disk structure. The light distribution suggests a centrally concentrated bulge with a gradual decline in brightness towards the outer regions. The core of the galaxy is bright and exhibits a yellowish-orange hue, potentially indicating an older stellar population. The galaxy's overall color suggests a lack of significant ongoing star formation. There is some minor unevenness in the light distribution, possibly hinting at a previous minor interaction, but the galaxy does not display any obvious signs of major disturbance or ongoing merger activity.
