The galaxy appears to be a relatively smooth, elliptical type. It presents a centrally concentrated luminosity profile with a fairly uniform color distribution. The central region exhibits a yellowish hue, suggesting a population of older stars. There are hints of a faint, diffuse halo surrounding the main body, but no distinct spiral arm structures or prominent dust lanes are discernible. The galaxy's overall shape is somewhat rounded, showing minimal elongation. There's no immediate visual evidence of ongoing major mergers or significant tidal disturbances, though subtle asymmetries might be present upon closer examination.
