The galaxy exhibits a generally smooth morphology, with a centrally concentrated, bright core. The light distribution appears elliptical, transitioning from a luminous, yellowish core to a fainter, more diffuse halo or envelope. The shape is more intermediate than distinctly round or elongated. There is little evidence of spiral arm structure or significant dust lanes. No signs of strong tidal interactions or ongoing major mergers are visible. There is a slight, faint blue or green tint to the outer region of the halo, possibly indicating some ongoing star formation. Overall, this galaxy appears to be a relatively undisturbed, evolved system.
