The galaxy presents as a diffuse, elliptical-like structure with a smooth overall appearance, but with some potential structure. It appears to be oriented at an angle relative to the line of sight. The central region exhibits a slightly brighter, more concentrated luminosity. The galaxy's color profile suggests a population dominated by older stars. There appears to be a suggestion of a disk, but it is difficult to assess its characteristics from the available data. There is a possibility of a minor disturbance in the galaxy's shape, but no major signs of an active merger. 
