The galaxy presents as a single, largely symmetrical object. The light is concentrated towards the center, forming a bright core. A relatively smooth light distribution is observed, decreasing in intensity from the center outwards. There are no obvious spiral arm structures or distinct disk features. The galaxy appears to be elliptical, with a predominantly round morphology. It does not seem to be undergoing any major merging events or tidal disturbances, and it doesn't show any signs of a strong active galactic nucleus. The color profile suggests a relatively older stellar population, with redder hues dominating.
