The galaxy presents a generally smooth and rounded morphology, indicative of an elliptical or lenticular type. The core exhibits a concentrated luminosity profile, appearing as a bright, nearly circular region with a yellow-orange hue. This central region is surrounded by a slightly fainter, more diffuse halo extending outward, which transitions into a bluish color. The overall structure lacks prominent spiral arms or significant dust lanes. There is no discernible evidence of ongoing major merging activity or tidal disturbances in the galaxy's immediate vicinity. The light distribution suggests a relatively high degree of radial symmetry.
