The galaxy exhibits a morphology consistent with an early-type spiral or lenticular galaxy, viewed at an intermediate inclination. It possesses a discernible bulge component that appears relatively smooth and concentrated, exhibiting a yellowish hue indicative of an older stellar population. The disk component, while present, is less prominent than the bulge, and appears bluer. There is no evidence of strong spiral arm structure. The overall shape is elongated, though not excessively so, and is considered somewhat round. There are no obvious signs of a major ongoing merger event, though a minor disturbance cannot be ruled out. The galaxy appears to be relatively isolated in this field.
