The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge exhibiting a yellowish hue. The surrounding disk appears relatively smooth and featureless, with a subtle flattening along one axis, suggesting it is not perfectly spherical. There is a very faint suggestion of a spiral arm structure or tidal disturbance on one side of the galaxy, but this is difficult to ascertain conclusively. The color gradient indicates a higher concentration of older stars in the bulge, while the disk likely contains a mix of stellar populations. There is no clear evidence of ongoing major mergers or significant starburst activity. The overall morphology suggests a galaxy transitioning toward an earlier type, possibly an early-type spiral or lenticular galaxy.
