The object presents as a relatively compact galaxy with a smooth, somewhat elliptical morphology. There's a dominant central bulge region exhibiting a bluish hue, suggesting a population of younger, hotter stars or ongoing star formation activity. This core is surrounded by a less defined, fainter halo. The overall color distribution indicates a possible mix of stellar populations, with the bluer colors concentrated in the central region and potentially older, redder stars contributing to the halo's color. There appears to be a slight asymmetry or disturbance in the outer regions of the galaxy, perhaps indicative of minor tidal interactions or past merger events. However, the overall structure doesn't show strong evidence of a recent major merger. The galaxy is not perfectly round, appearing slightly elongated.
