The galaxy presents as an elliptical morphology with a smooth, diffuse light profile. The central region exhibits a significantly higher luminosity, concentrated in a bright, compact core. The overall color is skewed towards the redder end of the spectrum, suggesting an older stellar population and a lower rate of star formation. The galaxy appears elongated, exhibiting a high degree of ellipticity. There is no readily apparent evidence of spiral arm structure or significant dust lanes. The outer regions gradually fade into the background, indicative of a decreasing stellar density with radial distance from the center. The general appearance suggests a relatively evolved system, possibly an early-type galaxy. There is some subtle clumping in the outer regions.
