This galaxy appears to be a late-type spiral galaxy, observed nearly edge-on. The disk is prominent, showing a higher degree of flattening. A bulge is also present, with a rounded shape and a significant contribution to the overall luminosity of the galaxy. There is a lack of evidence for a classical spiral arm structure, but minor disturbances might be present, perhaps the result of past interactions. The dominant colour is yellow-red, this could suggest the stellar population may be dominated by older stars. There is also a faint, diffuse halo or extended disk surrounding the main body of the galaxy. There is a significant concentration of light towards the central regions, indicating a high density of stars and potentially a supermassive black hole at the nucleus. I see no definitive signs of ongoing major merging activity.
