The galaxy presents a primarily smooth morphology, exhibiting a high degree of central concentration. Its overall shape appears generally elliptical, with a notable lack of distinct spiral arm structure. The galaxy's color profile suggests a relatively evolved stellar population, with a redder hue dominating the light emitted. There are minor asymmetries that indicate a slight interaction or disturbance. Evidence of recent or ongoing star formation is limited, although may exist within the core of the object. The galaxy shows some minor signs of tidal disturbances or past interactions, but it appears to be largely undisturbed.
