The galaxy presents as a spiral galaxy with a prominent, moderately sized bulge. There is evidence of a bar structure running through the center of the galaxy, with tightly wound spiral arms emerging from the ends of the bar and extending outwards. The arms are faint, with no clearly defined areas of star formation. The bulge appears to be composed of older stars. The galaxy has a slight disk-like structure but is viewed somewhat face-on. There are hints of weak dust lanes within the galaxy, primarily around the edges of the bulge. The overall color suggests a mix of stellar populations, but dominated by older stars. No signs of major disturbances or recent merger events are observed.
