The galaxy presents as a centrally concentrated object with a largely smooth morphology. The central region appears quite bright and unresolved in this imaging, exhibiting a moderate color temperature, tending slightly toward bluer wavelengths. This suggests the presence of a relatively old stellar population. The overall shape approximates a slightly elliptical, but more or less circular form. There is a hint of asymmetry in the outer regions, which might be indicative of past or ongoing minor gravitational interaction. No obvious spiral arm structure is visible. The galaxy is relatively compact, with a concentrated light profile. There may be subtle variations in color across the galaxy, but it is not possible to determine distinct sub-regions based on color alone. No strong signs of recent, intense star formation are evident from the image.
