The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is a bright yellowish-white color, indicative of an older stellar population. There is a slight elongation to the galaxy's shape, though it is mostly round. Fainter, diffuse blue light surrounds the central bulge, suggesting some presence of younger, star-forming regions within the galaxy's outer parts. The galaxy appears to be fairly isolated, showing no signs of significant tidal disturbances or ongoing mergers, though there might be a very slight asymmetry suggesting a minor past interaction. Overall, it presents as a fairly evolved system with an older stellar population dominating the central regions.
