The galaxy appears as a centrally concentrated elliptical-like structure with a smooth luminosity profile. The core exhibits a bright, yellowish-white hue, indicating a likely older stellar population. Moving outwards from the core, the galaxy's color gradually transitions to a more reddish tone, suggesting the presence of evolved stars and possibly a decrease in ongoing star formation in the outer regions. A faint disk is barely visible; it's slightly inclined relative to our line of sight. The overall form is well-defined. There seems to be no signs of active merging events or major tidal disturbances and the features are very smooth.
