The galaxy presents as a largely featureless elliptical galaxy with a high degree of central concentration, suggesting an older stellar population and a possible lack of significant dust lanes or active star formation in the inner regions. The light distribution appears smooth and symmetrical, with a slight elongation observed along an axis oriented approximately northwest to southeast. The galaxy core is bright and diffuse, exhibiting a yellow-red hue, suggestive of a population of evolved stars. The outer regions of the galaxy display a gradual decrease in surface brightness, indicative of a smooth stellar halo. There is no visible evidence of spiral arms, a bar structure, or any major disturbances that would suggest a recent merger event. The galaxy's overall morphology is consistent with an elliptical classification, characterized by its spheroidal shape and lack of prominent features.
