The galaxy presents as an elliptical morphology, exhibiting a smooth, spheroidal structure. The central region displays a high concentration of light, suggesting a significant population of older stars. There is little evidence of dust lanes or spiral arm structures. The color profile leans toward the redder end of the spectrum. A smaller, fainter object is visible in close proximity to the main galaxy. The object does not appear to be tidally disrupting the galaxy. The galaxy appears fairly isolated.
