The galaxy presents as a centrally concentrated, luminous object. It appears to be an elliptical galaxy, exhibiting a largely smooth morphology with minimal discernible features such as spiral arms or dust lanes. The galaxy's shape is somewhat elongated, approximating a prolate spheroid, with an intermediate ellipticity.

The galaxy's color profile suggests an older stellar population. The central bulge exhibits a yellow-orange hue, indicative of evolved stars, while the outer regions transition to a bluer color, possibly signifying the presence of a younger, albeit smaller, population of stars. There is no evidence of ongoing major merger activity or strong tidal disturbances. The smooth light distribution and lack of prominent features support the classification of this galaxy as an elliptical, with little ongoing star formation.