The galaxy appears as a moderately compact, elliptical or lenticular-like structure. It has a relatively smooth texture, with no discernible spiral arms or prominent dust lanes visible in the image. The light distribution seems relatively even across the galaxy, with a slight concentration towards the center. The overall color profile indicates a population of older stars, with a tendency towards redder wavelengths as indicated by the magnitudes, which may suggest a suppressed or declining rate of recent star formation. There is a hint of blue light at the upper area of the galaxy indicating some regions of star formation activity. Based on its shape, color, and relatively smooth appearance, the galaxy is likely a fairly evolved system. There appear to be small signs of disturbance around the galaxy which could indicate that the galaxy is undergoing or has undergone a minor merger event.
