The galaxy appears to be elliptical, exhibiting a smooth, spheroidal morphology with no discernible spiral arms or disk-like features. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. The galaxy is largely featureless, suggesting a relatively old stellar population. The color is slightly redder, implying that the stellar population is primarily composed of older, redder stars, with minimal ongoing star formation. There are no obvious signs of recent interactions or mergers, such as tidal tails or distorted shapes. The galaxy appears well-defined, lacking significant disturbances.
