The galaxy presents as a somewhat elongated, cigar-shaped structure. A smooth, centrally concentrated bulge is observed, exhibiting a yellowish-orange hue. The outer regions of the galaxy appear less defined and bluer in color, suggesting younger stellar populations within the galaxy. There is no evidence of spiral arms, but the disk appears weakly defined. The overall morphology suggests a galaxy undergoing star formation, though perhaps with a diminishing rate. The shape suggests the classification of an elliptical galaxy. There does not appear to be a major ongoing merger or any significant tidal disturbances.