The galaxy presents as an elliptical morphology, elongated in shape, with a smooth, featureless appearance. There is a concentration of light towards the center, with the luminosity gradually decreasing towards the outer edges. The color appears relatively uniform across the galaxy, with a slight blue hue, particularly in the central region. This suggests the presence of a population of relatively young, hot stars. The overall structure indicates a system dominated by an older stellar population, with little to no evidence of spiral arms or significant dust lanes. No apparent signs of major interaction or tidal disturbances are observed.
