The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology with a slight elongation. Its color profile suggests a population of older stars, with a noticeable absence of strong blue emission indicative of ongoing, high-rate star formation. The galaxy's light is concentrated towards the center, implying a possible central bulge component. A faint disk-like structure might be present, but is not well-defined in the image. There is a very slight asymmetry in the light distribution, hinting at a possible minor gravitational disturbance or past interaction, although there are no clear signs of tidal tails or significant morphological disruption. The system's apparent size indicates a mid-sized galaxy, and it appears relatively isolated in its environment.
