The galaxy presents as a luminous, centrally concentrated object. Its overall form appears elliptical with a high degree of central smoothness. There is a subtle halo of lower surface brightness extending outwards from the core, gradually fading into the background. A slight elongation is observed, deviating somewhat from a perfect circularity. Minimal internal structure is discernible; no prominent spiral arms or dust lanes are apparent. There is no clear evidence of any ongoing major merger activity, although some subtle asymmetries in the outer regions could indicate minor disturbances or past interactions. The galaxy's color is generally yellow, suggesting an older stellar population with a relatively low rate of on-going star formation.
