The galaxy appears as a smooth, elliptical structure. It exhibits a concentrated central bulge that gradually fades into a less defined outer region. The color profile suggests a relatively homogenous stellar population. There is little evidence of prominent spiral arms or significant dust lanes. The galaxy is elongated, but appears well-ordered with no major morphological disturbances. The overall light distribution suggests a system dominated by older stars, though the color implies some ongoing, though likely low, star formation.
