The galaxy presents a somewhat elliptical morphology, appearing as a flattened spheroid. Its central region exhibits a concentrated, bright core, suggesting a higher density of stars or an active galactic nucleus. Surrounding the core is a less defined disk, discernible through a gradual decrease in luminosity and a bluer hue. This disk appears relatively smooth, lacking prominent spiral arm structures. The overall color profile indicates a presence of both older, redder stellar populations in the core and slightly younger, bluer stars in the disk. The galaxy appears to be relatively isolated, showing no obvious signs of recent major merger activity, but there is a very slight distortion of the disk structure in the upper left, perhaps showing that there may have been minor disturbance in the galaxy's past. The galaxy is of moderate size.
