The galaxy presents a generally elliptical morphology. There is a prominent, centrally concentrated bulge region exhibiting a yellowish hue, likely indicative of an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component, with hints of bluer colors suggesting more recent star formation. The disk appears somewhat flattened, with a noticeable tilt relative to our line of sight. While there is no clear spiral arm structure immediately apparent, subtle irregularities in the disk's light distribution indicate possible underlying features. The overall smooth appearance of the galaxy points toward a relatively evolved system, with ongoing, but likely subdued, star formation activity. There appear to be some minor tidal disturbances present.
