This galaxy appears to be a relatively smooth, elliptical system. Its morphology suggests an older stellar population, with a centrally concentrated bulge that emits primarily in the yellow-red wavelengths. There's no visible dust lane or prominent spiral arm structure, indicating a lack of significant ongoing star formation. The galaxy appears quite symmetrical, with a slight elongation. It shows minimal signs of tidal disturbance or interaction with other galaxies. The outer regions gradually fade in intensity, which may indicate a large but diffuse halo component. Given the overall appearance, this galaxy is likely a fairly massive system that has undergone significant evolution.
