The galaxy presents as a moderately luminous, elongated structure. Its morphology appears largely smooth, with a high degree of central concentration in its light distribution. It has a color profile indicating an older stellar population and low ongoing star formation. The overall shape is intermediate between round and elongated, showing a lack of spiral arm structure or prominent disk features. There may be some evidence of tidal disruption in the faint outer halo, suggesting minor gravitational interactions with other galaxies, however no major mergers are ongoing.
