The galaxy presents a largely smooth morphology, appearing as a single, cohesive structure. There is a slightly elongated shape; it is not perfectly circular but leans towards being an elliptical galaxy. There is a bright central bulge that contributes strongly to the overall luminosity. Fainter, diffuse light extends outwards from this core. There are very subtle hints of possible disturbances in the galaxy's form, which may indicate a past or ongoing interaction with another galaxy. There is no clear evidence of spiral arm structure or prominent dust lanes within this galaxy.
