The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge that appears nearly circular in projection. The light distribution suggests a centrally-dominant spheroid. There's a noticeable radial color gradient, with the core appearing bluer than the outer regions. The galaxy shows no prominent spiral arms, bars, or other obvious disk features, which further supports a classification as an elliptical. The galaxy's overall morphology indicates a system that is likely dynamically relaxed, potentially the result of past merger activity. There is no apparent indication of strong tidal interactions with neighboring galaxies or a significant amount of ongoing star formation in the outer regions.
