This galaxy presents as a roughly elliptical object with a bright, concentrated central region, most likely a galactic nucleus. The central brightness suggests a significant amount of active star formation or possibly the presence of an active galactic nucleus. Surrounding this bright core is a more diffuse and fainter outer region. The overall color profile suggests a higher concentration of younger, bluer stars in the central area, while the outer regions exhibit a slightly redder hue, which could indicate an older stellar population. There are faint disturbances to the morphology, suggesting a possible past or ongoing interaction or merger with another galaxy. The overall structure appears relatively smooth, but the slight irregularities indicate some level of dynamical activity.
