The galaxy presents as a disk galaxy, viewed at a moderate inclination. The central bulge appears prominent and smoothly luminous, indicating a significant population of older stars. The disk component is less distinct, with a gradual transition in color and brightness from the bulge outwards. There are some faint traces of spiral arm structure, although they are poorly defined, suggesting either a flocculent spiral or a spiral galaxy with arms that are being disrupted. The galaxy's overall color is relatively red, indicative of a relatively low rate of star formation and a dominant population of older stars. The shape of the galaxy appears somewhat elongated, rather than perfectly circular, though this could be due to the viewing angle. There is no obvious presence of dust lanes or strong star-forming regions within the galaxy. There is no obvious evidence of interaction with neighboring galaxies or significant morphological disturbances.
