This galaxy appears to be a relatively compact object, showing a distinct central bulge region. This bulge is bright and concentrated, possibly indicating a high density of older stars. Moving outward from the central bulge, there appears to be a surrounding disk component, although its features are not well-defined. The disk is noticeably bluer in color compared to the bulge, suggesting the presence of younger, hotter stars and potential ongoing star formation. The overall shape of the galaxy is somewhat elliptical, with the disk seemingly tilted at an angle relative to our line of sight. There might be some very minor tidal disturbances or asymmetries.
