The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. Its color profile suggests an older stellar population, exhibiting a yellowish-orange hue that indicates a relative paucity of ongoing star formation. There is no discernible spiral arm structure or prominent dust lanes. The overall shape appears largely spheroidal, though a subtle elongation may be present. No signs of significant tidal disturbances or interactions with other galaxies are apparent in this image. The galaxy's light is dominated by older stars, and has very little star formation occurring.
