The galaxy presents as a roughly elliptical structure with a smooth, centrally concentrated luminosity profile. There is little evidence of spiral arm structure or significant dust lanes, suggesting it is not a spiral galaxy. The color gradient indicates a relatively older stellar population, with a yellowish-white core that transitions to a slightly redder halo. The galaxy appears to be relatively undisturbed, without any obvious signs of ongoing major merger activity or tidal distortions. It seems to be an isolated galaxy, with no obvious interacting companions.
