The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that dominates the overall luminosity. The color gradient suggests a slightly redder center, likely indicating an older stellar population. The outer regions appear fainter and subtly bluer, potentially hinting at some presence of younger, star-forming regions, although the overall color is still on the redder side. The galaxy's shape is elongated, exhibiting a flattening ratio of approximately 0.7, with a major axis oriented at approximately 30 degrees relative to the image's horizontal axis. There is a possible minor disturbance in the galaxy's morphology, with an area of asymmetrical light distribution. The light from the galaxy is consistent with a redshift of approximately 0.12, indicating a substantial distance.
