The galaxy presents as a slightly tilted disk with an overall elliptical shape. The central region exhibits a high surface brightness, appearing more concentrated and yellowish-white in color, likely indicating a significant population of older stars. Moving outwards from the center, the galaxy's color transitions to a bluer hue, suggesting the presence of younger stellar populations in the outer disk. There are no clearly defined spiral arms visible; the light distribution seems relatively smooth and diffuse. The galaxy exhibits a notable degree of flattening, as evidenced by the ratio of its minor to major axis. There is no apparent presence of significant dust lanes or irregular features, indicating that the galaxy is not undergoing major interactions or disturbances.