The galaxy presents as a slightly elongated, luminous object with a concentrated central bulge. The light profile suggests a smooth distribution, transitioning gradually from the bright core to a less intense halo. While the galaxy does not exhibit strong spiral arm structures, there are hints of a faint, extended disk surrounding the central region. The color appears to be a yellowish-orange, indicating a potentially older stellar population, particularly in the bulge. There are no obvious signs of active galactic nuclei or intense star formation regions within the central area from this image alone. The overall impression is of a relatively mature galaxy, possibly a lenticular or early-type spiral undergoing a period of quiescence.
