The galaxy appears to be an elongated spheroid in shape, possibly a lenticular or elliptical type. It has a smooth overall appearance with a concentration of luminosity toward the center, suggesting a substantial bulge component. The color gradient transitions from a yellow-white core to a bluer periphery, indicative of potential variations in stellar populations. There are no clearly defined spiral arms or prominent dust lanes visible. The galaxy doesn't appear to have any major disturbances or signs of ongoing merger activity, though there is a faint asymmetry in its outer regions, suggesting possible minor interaction in the past. The colors indicate some ongoing star formation, though not at a high rate.
