The galaxy presents an overall elliptical morphology, appearing as a somewhat flattened spheroid. The core region exhibits a concentrated luminosity with a yellowish-white hue, indicative of an older stellar population. A subtle disk-like structure is suggested by the slightly flattened appearance and the extension of the galaxy's light along a particular axis. A faint blueish-green tint is observed in the outer regions of the galaxy, potentially indicating ongoing star formation activity, although it appears somewhat subdued. There are no clear signs of spiral arms or prominent dust lanes. The overall texture is smooth, with no obvious signs of recent major merger events or significant tidal disturbances. The galaxy appears relatively isolated.
