This galaxy presents as a largely smooth, centralized mass of light. There is a somewhat elongated shape, appearing mostly round, but it is somewhat cigar shaped. The central region exhibits a bright, concentrated core, fading into a yellowish, extended halo, which is indicative of an older stellar population. The light distribution appears relatively uniform, with a high fraction of the light concentrated in the bulge, as expected in older galaxies. There are hints of a faint, diffuse disk, but no clear spiral arm structures are discernible. I see no evidence of any major tidal distortions or ongoing mergers, minor disturbances possible, as I can see asymmetry in the halo light surrounding the central core. There may be some possible signs of minor merger activity or internal disturbances. Based on its color and morphology, this galaxy is possibly an elliptical galaxy.
