The galaxy presents a generally smooth morphology with a notable lack of distinct spiral arm structures. It exhibits a pronounced central bulge that appears elongated, giving the galaxy an overall cigar-like shape. The color profile suggests a relatively old stellar population, indicated by the redder hues concentrated in the bulge. A faint disk is visible, although it is not clearly resolved into distinct features. The overall structure suggests this galaxy is likely an elliptical or lenticular galaxy, undergoing minimal current star formation. There is no evidence of any recent major merger events or significant tidal disturbances.
