The galaxy presents as an elliptical morphology, appearing generally smooth and well-defined. It exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually towards the outer regions. The core displays a yellowish hue, which may indicate a population of older stars dominating the central region. The shape of the galaxy is mostly round, only slightly elongated. There is no evidence of prominent spiral arms or a distinct disk structure. Based on the surrounding environment, there is no immediate interaction or merging activity with other galaxies visually apparent. There is a slight blueish hue to the outer halo of the galaxy, which could indicate more recent star formation.
