The galaxy presents as a relatively bright object with a smooth morphology, with the bulk of light exhibiting a somewhat elliptical distribution, though it tends toward being roundish. There may be a very subtle disk-like structure present, but no distinct spiral arms are discernable. The galaxy is largely devoid of prominent features such as dust lanes or strong star-forming regions, with the color being relatively uniform across the galaxy's body. There is no indication of any ongoing major merger events, nor any major disturbances to the overall structure. The light is concentrated, but not exceptionally so. The luminosity suggests a galaxy of considerable mass, with relatively low star formation activity.
