The galaxy exhibits a generally smooth morphology, with a slightly elongated shape, suggesting it might be classified as an elliptical galaxy or potentially a lenticular galaxy viewed at an angle. The central region displays a high concentration of light, indicating a prominent galactic bulge. The outer regions of the galaxy appear fainter, with a gradual decrease in luminosity away from the center. There is a subtle hint of a disk-like structure, but it is not well-defined. The galaxy appears to be relatively isolated, without any obvious signs of major interaction or recent merger events. The color profile is relatively uniform across the galaxy, with a slight tendency toward redder hues, indicative of an older stellar population and relatively low levels of on-going star formation. There may be evidence of minor disturbances in the form of faint tidal tails, but this requires further investigation with higher resolution imaging. Overall, the galaxy presents a picture of a well-evolved system with a dominant bulge component and potentially a weak disk component.
