The galaxy presents an elongated, elliptical morphology with a noticeable central bulge. The central region exhibits a bright, concentrated luminosity, suggestive of a dense stellar population, possibly an older population. Moving outward from the core, the luminosity gradually decreases. The outer regions appear less defined, with a smoother texture and a blueish hue, potentially indicative of more recent star formation activity. There is a hint of a disturbed structure, possibly from a minor merger event. The overall color profile implies a mix of stellar populations, ranging from older, redder stars in the core to younger, bluer stars in the outer regions. The galaxy appears relatively smooth, without prominent spiral arms or significant dust lanes visible in this imaging. The image suggests it has a moderate degree of flattening.
