The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The color profile is dominated by redder hues, suggesting an older stellar population with minimal ongoing star formation. There are no apparent spiral arm structures or significant dust lanes visible in the image. The overall morphology indicates a lack of recent major mergers or tidal disturbances. The galaxy exhibits a compact form, indicating a relatively high mass concentration within its central region. The light distribution appears uniform, lending to the classification as an early-type galaxy.
