This galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. The core region exhibits a high surface brightness, indicating a concentrated stellar population. Moving outwards, the galaxy's light gradually diminishes, forming an extended halo. A subtle disklike feature is apparent. The color profile suggests a relatively old stellar population, with a general redder hue, but with indications of some star formation. Possible tidal features are present, as minor disturbances are suspected. Overall, the galaxy seems to be generally isolated, not exhibiting strong interactions with other galaxies in the immediate vicinity.
