The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. The overall shape appears to be generally rounded, with a slight elongation. There is no significant presence of spiral arms or a well-defined disk.

The galaxy's core exhibits a bright, concentrated region, indicating a high stellar density. The color distribution is fairly uniform, with a yellowish hue across the visible spectrum. The yellow indicates there are older populations of stars within the galaxy. This is further substantiated by low star formation rates.

There is no significant evidence of recent major mergers or tidal disturbances in the image, though subtle asymmetries and disturbed regions are present, which suggests a potential minor interaction with another galaxy or internal dynamical processes.
