The galaxy presents a centrally concentrated luminosity profile, exhibiting characteristics consistent with an elliptical morphology or potentially a lenticular galaxy viewed at a shallow inclination. The central bulge is noticeably prominent and appears yellowish-red. A faint disk-like structure or extended halo surrounds this central region, appearing bluish due to probable star formation regions. The galaxy does not present any strong evidence of ongoing major mergers or tidal interactions, although some faint irregular structures are suggestive of minor disturbances. The galaxy is reasonably symmetrical, with no dominant spiral arms or other obvious features typically associated with late-type spiral galaxies. Overall, it appears to be a galaxy with a mature stellar population, possibly experiencing low levels of ongoing star formation within its disk or halo.
