This galaxy presents as a relatively smooth, elliptical structure. The core exhibits a concentrated, yellowish-white luminosity, suggesting a significant population of older stars. The overall shape appears slightly elongated, but predominantly round. Faint blue-ish wisps are seen sparsely distributed in the outer regions of the galaxy, hinting at very subdued star formation activity. There is no clear evidence of a spiral structure, or any major disturbances like tidal tails or prominent asymmetries. The galaxy is mostly isolated with no signs of interaction or merging with other galaxies.
