The galaxy exhibits a primarily elliptical morphology with a slight degree of flattening. The central region is dominated by a bright, concentrated bulge showing a yellowish hue suggesting an older stellar population. The galaxy appears to have an extended halo or disk component, which is fainter and bluer. A small degree of asymmetry is apparent in the outer regions, possibly indicative of minor gravitational interactions. Dust lanes are not clearly observed within the disk, suggesting a relatively smooth distribution of stellar material.
