The galaxy presents as a somewhat rounded, centrally concentrated object. Its morphology appears largely smooth, with a notable lack of distinct spiral arms or other prominent features typically associated with disk galaxies. The central region exhibits a bright, condensed core that gradually fades into the outer regions. The galaxy displays a yellow-red color profile overall, suggesting an older stellar population with relatively low ongoing star formation, which is consistent with an elliptical classification. There is no obvious evidence of significant tidal disturbances or ongoing mergers. The image quality suggests a relatively distant object where finer details are not easily discernible.
