The object appears to be a galaxy, generally elliptical in shape when considering its overall light distribution. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a galactic bulge. Moving outwards from the center, the light fades gradually, transitioning to a fainter halo. A faint disk structure is visible, characterized by a slight flattening of the galaxy's profile, oriented roughly horizontally in this image. There is some indication of minor disturbance in the galaxy's structure. This disturbance is faint. The lack of obvious spiral arms or prominent dust lanes points towards a classification as either an elliptical galaxy or a lenticular galaxy. Further spectroscopic analysis is needed to fully determine the galaxy's composition, age, and distance.
