The galaxy presents as a lenticular or possibly a spiral galaxy viewed at a high inclination. The overall shape is elongated with a bright, concentrated central bulge. The disk component appears relatively smooth and featureless, with no prominent spiral arm structures readily discernible. The color gradient suggests a population of older stars, with the central bulge exhibiting a yellowish hue. The disk appears slightly bluer than the bulge, implying a small level of ongoing star formation. There is no apparent evidence of significant tidal distortions or ongoing major mergers. There might be some minor disturbances in the disk, but that is uncertain given the image resolution. The galaxy does not appear to be actively forming large numbers of stars, and it shows no signs of an active galactic nucleus.
