The galaxy presents as a centrally concentrated system with a generally elliptical morphology. It exhibits a smooth light distribution with a subtle extension towards the upper right. The core is well-defined, exhibiting no obvious signs of active galactic nuclei. There is no prominent disk structure, spiral arms, or bar visible. The galaxy appears to have a yellowish-red hue, suggestive of an older stellar population, potentially indicating that star formation activity is low. Evidence of potential interaction or recent merger is present, evidenced by an overall disturbed morphology.
