The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, with light gradually diminishing towards the outer edges. There is a slight elongation to the galaxy's shape; it is more 'in-between' than perfectly spherical. The color profile indicates a population of older stars, with a distinct lack of blue light, suggesting low recent star formation. There are no apparent spiral arm structures or significant dust lanes visible within the image. Overall, the galaxy appears to be a well-defined, isolated system, showing no obvious signs of major interaction or merging with other galaxies, although there may be minor disturbances.
