The galaxy appears as a centrally concentrated, luminous object with a roughly elliptical morphology. The central region exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. The isophotes are generally smooth, with a high degree of central concentration. Fainter, bluer extensions are visible to the top and left sides. The overall structure suggests a relatively evolved system with a minimal amount of ongoing star formation. There are no prominent spiral arms or strong dust lanes visible in the image. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal interactions. There is a slight asymmetry in the faint outer regions.
