The galaxy presents as a moderately luminous elliptical, exhibiting a smooth, concentrated morphology. The central bulge is prominent and appears near-spherical, displaying a yellow-orange hue, indicative of an older stellar population. The isophotes show some elongation with a major axis oriented approximately northwest to southeast. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or recent mergers in this field of view. Faint blue regions are distributed within the galaxy's extended halo, which could represent regions of low star formation. The lack of prominent spiral arms or dust lanes suggests a classification towards the early-type end of the galaxy sequence.
