The galaxy presents as a generally smooth, elliptical morphology. The core exhibits a concentrated luminosity, suggesting a high stellar density in the central region. Fainter, diffuse light extends outwards from the core, forming a halo structure. There is a slight elongation in the galaxy's shape, hinting at a possible deviation from a perfectly spherical form, but it is mostly rounded in appearance. No distinct spiral arms or prominent dust lanes are discernible within the image. The galaxy does not appear to be undergoing any major merging events or strong tidal interactions with other galaxies, although there may be minor disturbances in the galaxy. Overall, the galaxy appears to be a relatively undisturbed, evolved system, with limited ongoing star formation activity. The color profile indicates a population of older stars.
