The galaxy presents as a somewhat elongated, elliptical structure. Its central region exhibits a concentrated luminosity, appearing smooth and relatively featureless. Moving outwards from the core, the intensity of light gradually diminishes. There is a hint of disklike-ness to the outer regions. The color profile is characterized by a yellow-reddish hue near the center, possibly indicating an older stellar population. Overall, the galaxy seems to be in a somewhat isolated environment, with no obvious signs of active merging events or major tidal disturbances, though some minor interaction cannot be ruled out due to the irregular outer shape.
