The galaxy presents a structure that appears largely smooth, with a possible slight elongation. The color profile suggests a relatively mature stellar population, with a bias towards redder hues. There are indications of some disturbed morphologies, possibly minor tidal features or asymmetries, which might point towards past or ongoing interactions. The central region seems to have a higher concentration of light. The galaxy is relatively compact. Some faint extensions or diffuse light might be present. Overall, the galaxy seems to be an early-type galaxy exhibiting some signs of disturbances.
