The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a relatively smooth, elliptical morphology. The light distribution suggests a prominent bulge component dominating the overall structure. The central region is significantly brighter and appears yellow, indicating a high concentration of older stellar populations. The galaxy disk, if present, is faint and difficult to resolve, showing a minimal amount of distinct spiral arm structure. There is a slight flattening and elongation of the galaxy's shape, suggesting it may not be perfectly spherical, but more cigar-shaped. There's no readily apparent evidence of ongoing major merger activity or significant tidal disturbances affecting the galaxy's structure. Faint blue regions might be present in the outer parts of the galaxy, indicating sparse regions of younger, hotter stars. The absence of prominent dust lanes and strong star formation regions supports its classification as an early-type galaxy with a relatively quiescent star formation history.
