The galaxy presents as a relatively compact object, likely an elliptical. The light distribution appears smooth and centrally concentrated, with a gradual falloff in intensity towards the outer regions. Its shape is generally rounded, lacking any obvious spiral arm structures or bar features. There is a hint of a disk-like structure, but not significant.

The galaxy displays a subtle color gradient. The core appears slightly bluer compared to the outer regions, which exhibit a redder hue. This may suggest the presence of a younger stellar population in the central area, or possibly ongoing star formation, though at a low rate. There is no obvious dust lane or tidal feature, indicating no major merging occurring. The redder outer colors suggest that the object has older stars.
