The galaxy presents a primarily smooth morphology, appearing largely spheroidal. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus, although no distinct jet or point source is discernible in this image. There is a slight elongation along one axis, indicating a possible deviation from a perfectly spherical shape, though it mostly has a rounded profile. Faint, diffuse structures appear adjacent to the main body of the galaxy, possibly representing tidal debris or extended stellar halos, but do not suggest a major ongoing merger. The galaxy's colour profile appears redder than that of typical spiral galaxies, possibly suggesting an older stellar population, reduced star formation or obscuration by dust.
