This galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core is a yellowish-orange hue, suggesting an older stellar population. The galaxy exhibits a slight elongation, tending toward a cigar shape, as opposed to being perfectly spherical. There is no clear indication of spiral arms or significant dust lanes. The overall structure appears relatively undisturbed, with no major signs of ongoing merging activity. A faint blue tinge on the edges suggests the presence of a small population of younger, bluer stars at the outer regions, with a possible low rate of star formation. Overall, this galaxy appears to be a mature system with a dominant population of evolved stars.
