The galaxy presents as an elongated, elliptical morphology. Its color profile indicates a dominant population of older stars, with a centrally concentrated yellowish hue. There is little indication of active star formation regions or prominent spiral arms within the visible structure. The galaxy appears relatively smooth with a high degree of central concentration. Slight irregularites appear on the edges of the galaxy. No signs of interaction, tidal tails, or significant disturbances are visually apparent. The overall impression is that of a mature, relatively undisturbed system.
