This galaxy appears to be a relatively smooth, elliptical system. It exhibits a generally round morphology, with minimal discernible disk-like features or spiral arms. The light profile suggests a high degree of central concentration, typical of elliptical galaxies. There is a pronounced color gradient, with a yellowish-white core indicative of an older stellar population, surrounded by a slightly bluer halo. This hints at some degree of recent star formation activity in its outer regions, though on a scale significantly lower than typically observed in spiral galaxies. There are no signs of any major merging activity or significant tidal disturbances. The overall impression is that of a well-evolved system.
