The galaxy presents as a relatively smooth, elliptical-like structure with a faint, diffuse outer envelope. The central region exhibits a slightly brighter concentration of light, indicative of a possible galactic nucleus. The galaxy appears to be an intermediate shape between round and elongated, lacking any distinct spiral arm features or prominent dust lanes. A subtle blue-ish hue is observable in the galaxy’s disk region, possibly indicating regions of recent star formation. No obvious signs of a major merger event or significant tidal disturbances are apparent.
