The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and concentrated light profile. There is little evidence of spiral arms. The central region is noticeably brighter than the outer regions, suggesting a significant concentration of stars. The galaxy appears slightly elongated, with the major axis oriented roughly horizontally in the image. There is some suggestion of a disk-like component to the galaxy, but this feature is not pronounced. The galaxy appears to be somewhat isolated, with no obvious tidal features or interactions with nearby galaxies visible in this image. The overall color appears relatively red, consistent with an older stellar population and low star formation rate. There is a hint of blue in the peripheral regions, potentially indicating some regions of younger stars or ongoing star formation in the outer disk.
