The galaxy appears to be an elliptical galaxy, classified as smooth and rounded, with a notable absence of spiral arms or a prominent disk structure. The light profile is centrally concentrated, indicating a higher density of stars toward the galactic center. There is a smooth, gradual fading of light intensity from the center outwards.

The color index suggests a relatively older stellar population, which is consistent with the lack of visible star formation regions. The galaxy's overall structure appears undisturbed, with no signs of ongoing major merger events or significant tidal interactions. There are subtle indications of minor asymmetries in the outer regions, possibly due to a minor disturbance, but the overall morphology remains largely undisturbed.
