The galaxy presents as a generally smooth and centrally concentrated object. Its overall morphology appears elliptical or spheroidal, lacking any obvious spiral arm structures or a prominent disk. The light distribution is relatively uniform, with the brightest region located at the galaxy's core, gradually fading towards the outer edges. The galaxy exhibits a moderate redshift, indicating a significant distance and lookback time. 

The color profile suggests a population of older stars, as indicated by the dominant reddish-yellow hue, particularly towards the galactic center. Some bluer tints can be seen in the outer edges of the galaxy. This could be attributed to some ongoing, albeit low level, star formation. There are no apparent signs of a major ongoing merger or significant tidal disturbances, though subtle irregularities hint at a possible minor interaction in the galaxy's past. The galaxy appears somewhat large in size, and the light is moderately bright. 
