The galaxy presents a somewhat elliptical morphology, appearing largely smooth and lacking distinct spiral arm structures. It exhibits a concentrated central bulge region with a bright, yellowish hue, suggesting an older stellar population. The outer regions of the galaxy display a gradual decrease in surface brightness, with a bluer tint that could indicate the presence of ongoing star formation, although not particularly vigorous. There is a slight elongation to the galaxy's shape, but no clear signs of major tidal disturbances or ongoing mergers are immediately apparent. The overall appearance suggests a relatively evolved system, possibly an intermediate-type galaxy between a spiral and an elliptical.
