The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The overall color profile suggests a mix of stellar populations. The central region exhibits a yellowish hue, possibly indicating older, redder stars. Moving outwards from the core, a bluish tint becomes more prominent, particularly in the extended disk region. This could suggest ongoing star formation activity in the outer regions. There are only faint hints of spiral arm structure, potentially disrupted or smoothed out over time. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The edges of the galaxy fade gradually into the background sky, which is indicative of a smooth stellar distribution.
