The galaxy presents as a single, moderately bright object with a noticeable central concentration of light. The morphology appears to be generally smooth and elliptical, with a slightly elongated shape and a lack of defined spiral arm structures. There's an indication of a central bulge, brighter than the surrounding disk, that diffuses outward into a fainter, more extended halo. The galaxy's color profile suggests a mix of stellar populations, with a redder hue in the central regions potentially indicating older stars, transitioning to bluer tints in the outskirts, suggesting younger stars. There might be a minor gravitational interaction or disturbance visible, given the slight asymmetry in the galaxy's halo. Overall, the galaxy appears relatively undisturbed.
