The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a somewhat rounded morphology. A prominent, bright central bulge is observed, displaying a yellowish-orange hue. This suggests a population of older stars dominating the core.  A fainter, bluer region is visible extending from the main body of the galaxy. This could be a tidal tail caused by a past or current merger event, or it could be a region of lower density with star forming regions. There appears to be some morphological disturbance, indicated by the irregularities present in the faint extension. It is possible that this galaxy is undergoing a merger or has experienced a recent interaction with another galaxy. The overall color profile suggests a galaxy transitioning towards a redder color, which can be typical of galaxies with reduced star formation.
