The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. Its overall shape appears elliptical, tending toward round rather than highly elongated. The core exhibits a brighter luminosity, indicative of a higher stellar density or possibly an active galactic nucleus, though no distinct point source is visible. Moving outwards from the core, the intensity gradually decreases into a faint halo region. There are no immediately apparent spiral arm structures or significant dust lanes within the visible light, although there appears to be a slight color gradient within the central region. The galaxy appears relatively isolated, showing no obvious signs of major mergers or strong tidal disturbances in its immediate vicinity. The galaxy's light is slightly blue in color, suggestive of some level of recent star formation, but generally appears to be an older and relatively relaxed stellar population dominating the light output.
