The galaxy presents as a centrally concentrated elliptical type, with a smooth, diffuse light profile. The core exhibits a yellowish-orange hue, suggestive of an older stellar population. Proceeding outward from the center, the color transitions subtly to a slightly bluer hue, particularly at the apparent edges, hinting at the presence of a younger stellar population. The galaxy’s overall shape deviates moderately from a perfect sphere, appearing somewhat elongated or cigar-shaped. There is no clear evidence of spiral arms or significant dust lanes within the galaxy. Minor irregularities are visible in the galaxy, perhaps indicating a minor interaction.
