The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge. The luminosity appears to decrease gradually from the core to the outer regions, suggesting a relatively smooth distribution of stars. There is a slight flattening of the disk, hinting at the presence of a disk component, though it is not particularly prominent. No distinct spiral arm structures are discernible within the limits of the image resolution, and there are no prominent dust lanes visible. The color distribution seems relatively uniform, indicating a generally older stellar population. The galaxy appears isolated, with no evident signs of tidal interactions or ongoing mergers. The overall impression is that of a quiescent, relatively evolved system.
