The galaxy presents a roughly elliptical morphology, appearing relatively compact. The central region exhibits a high surface brightness, indicative of a concentrated core. The galaxy appears to show some degree of disturbance, with a slight asymmetry in its overall shape.  There is a faint indication of tidal features or faint arm-like structures extending from the main body.  The color profile suggests a predominantly older stellar population, with a significant redder component.  There is also a notable blue component concentrated within the core and inner regions, potentially indicating ongoing or recent star formation.  The galaxy does not appear to be strongly interacting with any other nearby galaxies in the immediate field.
