The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be moderately inclined relative to our line of sight. The central region exhibits a bright, concentrated core, suggesting the presence of an actively star-forming region or possibly an active galactic nucleus. The light distribution fades gradually from the core outwards, with no prominent spiral arm structures visible. The overall color of the galaxy is slightly reddish-yellow, which suggests an older stellar population. No obvious signs of recent major merging activity are apparent, although some minor disturbances in the outer regions may be present. The galaxy's shape appears to be somewhat elongated, with an estimated diameter of around 6 kpc.
