The galaxy appears as a single, concentrated object with a generally smooth profile. There is a slight elongation, but the shape is mostly rounded. The color profile indicates a population of stars that is relatively homogenous and a small amount of on-going star formation is estimated. There are no obvious signs of a major merger, although a slight disturbance could be present. The galaxy exhibits a redder color in the central regions, with a color gradient towards bluer hues in the outer reaches. The structure shows no distinct features, such as spiral arms or a prominent bar. The galaxy’s overall appearance suggests a morphological type that leans toward a spheroidal galaxy, possibly an elliptical or S0.
