The galaxy appears as a centrally concentrated elliptical system. It exhibits a smooth, diffuse light profile, lacking prominent spiral arms or a distinct disk. There is a slight elongation to the galaxy's shape, deviating from a perfectly circular morphology. The core region shows a brighter, more intensely colored light, indicating a higher density of stars. Fainter, more diffuse light extends outward from the core, gradually fading into the background. There are suggestions of minor irregularities in the outer regions, which may indicate possible disturbances from past interactions with neighboring galaxies, but is difficult to tell. The galaxy displays an apparent red color, suggesting an older stellar population and ongoing star formation.
