The galaxy presents as a luminous, moderately sized system with an overall elliptical morphology. The central region exhibits a concentrated, bright, yellowish-orange core, potentially indicating an older stellar population or the presence of a supermassive black hole actively accreting material.

Surrounding the core, a more diffuse, fainter halo of light extends outwards. This outer region appears bluer in hue, suggesting the presence of younger stars or ongoing star formation, albeit at a relatively low rate. The galaxy's overall appearance is somewhat smooth, though subtle irregularities in the outer regions hint at possible past interactions or minor disturbances, but overall a rather relaxed morphology. There is little evidence of strong tidal features or ongoing major mergers. The galaxy is more akin to a somewhat relaxed and mature object.
