The galaxy presents a largely smooth morphology, with a high degree of central concentration. The light distribution suggests an elliptical or lenticular galaxy type, displaying a somewhat rounded shape. There is a noticeable color gradient, with the central region exhibiting a yellowish hue, potentially indicative of an older stellar population, while the outer regions show slightly bluer tones, possibly pointing towards a younger, though not particularly active, stellar population. No significant signs of ongoing mergers or major disturbances are visible in the image. The galaxy appears to be fairly isolated. Based on the observed characteristics, this galaxy could be a relatively massive early-type galaxy with a suppressed star formation rate.
