The galaxy presents as a largely smooth, centrally concentrated object. Its morphology appears elliptical, with a high degree of symmetry. Color gradients suggest a relatively older stellar population, with the core exhibiting a yellowish hue indicative of evolved stars. There is a subtle decrease in surface brightness moving outward from the center. The galaxy does not show any obvious signs of spiral arms, prominent dust lanes, or active star-forming regions. There might be very faint hints of a disk but this is uncertain. There is no evidence of tidal tails or other morphological distortions that would suggest a recent major merger. The galaxy is approximately 7 kiloparsecs in radius and the mass is approximately 10^10.75 solar masses. The star formation rate is low.
