The galaxy presents an overall elliptical morphology, though it is slightly elongated. A prominent central bulge is evident, appearing bright and concentrated, with a yellowish hue indicative of an older stellar population. This bulge seems to gradually fade into a more diffuse surrounding disk. Some evidence of a disk component is present, albeit lacking well-defined spiral arms. The overall color suggests a mix of stellar populations, with the bulge showing older stars and the disk potentially harboring some younger, bluer stars, although this is difficult to confirm with certainty from the image. There may be a very slight tidal disturbance or asymmetry present, but the general structure of the galaxy appears largely undisturbed.
