This galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round with only a slight elongation. The galaxy's light profile transitions smoothly from a bright, dense core region outwards. The core exhibits a yellowish hue, which suggests a population of older stars. Moving outwards from the center, the color shifts towards a slightly redder tone, but there is little evidence of significant blue light indicative of active star formation. Faint outer regions suggest the presence of a diffuse halo. There's no visible evidence of spiral arms, bar structures, or major disturbances indicating a recent merger event, though there may be some minor irregularities in its overall shape. Overall, the galaxy appears to be a passively evolving system.
