The galaxy presents as a slightly elongated, diffuse structure. It appears to have a prominent central bulge, exhibiting a concentrated, yellowish-orange hue. Surrounding the bulge, a fainter, more extended disk-like component is visible. This outer region shows a mottled texture, potentially indicative of active star formation regions. The overall color suggests a significant population of older stars, although the hints of bluer regions indicate ongoing, albeit perhaps moderate, star formation activity. There are some signs of minor disturbance in the galaxy's structure, possibly hints of past or ongoing interactions with other galaxies, though no strong merging activity appears to be currently occurring.
