The galaxy presents as an elongated, elliptical structure. The central region exhibits a high degree of luminosity, appearing significantly brighter than the outer regions. Moving outwards from the core, the light intensity gradually diminishes. The galaxy has a smooth appearance overall with what appears to be a bulge. There is faint bluer light indicating it is a disk galaxy with some star formation. It does not display any clear signs of ongoing major merging activity or tidal disturbances. Its shape is more elongated than circular. The light from this galaxy indicates the bulk of the galaxy's stars are older, however some star formation is present.
