The galaxy presents as a centrally concentrated elliptical morphology. The core exhibits a high degree of luminosity, suggesting a dense stellar population and potentially an active galactic nucleus. A smooth, diffuse halo surrounds the central region, fading into the background sky. There is little evidence of spiral arm structure or distinct dust lanes. The overall color appears yellowish-white, consistent with an older stellar population dominated by redder giant stars. The apparent lack of significant blue light suggests a relatively low rate of ongoing star formation. The galaxy appears relatively undisturbed, without obvious signs of tidal interactions or major mergers.
