The galaxy presents as an elliptical morphology, appearing cigar-shaped. It exhibits a smooth, relatively featureless profile, suggesting an older stellar population. The central region is brighter and yellowish in color, indicative of a concentration of evolved stars. A fainter, more diffuse halo surrounds the core, extending along the major axis. There is no clear evidence of spiral arms or a prominent disk structure. The color gradient suggests a modest amount of ongoing star formation. There are no obvious signs of recent major merger activity or significant tidal disturbances in the galaxy's structure.
