The galaxy presents as a fairly compact, elliptical-like system. The light distribution appears smooth and centrally concentrated, lacking any obvious spiral arm structures or prominent disk features. There is no obvious indication of a recent major merger or tidal disturbance. The color gradient is subtle, with a central region exhibiting slightly yellower hues, potentially indicative of an older stellar population. The overall light profile is relatively uniform and symmetrical. There is a marginal possibility of minor irregularities in the light distribution at its periphery, however. It appears relatively isolated within its immediate surrounding field, with no close companion galaxies or obvious signs of interaction.
