The galaxy presents as a somewhat elliptical, though nearly round, extended object. There is a bright, concentrated central bulge that appears smooth and largely featureless in this image. Diffuse light extends outwards from the central region, fading into the background. The colors suggest a population of relatively old stars, with a hint of bluer light in the outer regions potentially indicating some ongoing star formation. There's no strong evidence of spiral arm structure or significant dust lanes visible at this resolution. There might be a slight irregularity or minor disturbance on one side, but it's not distinctly indicative of a major merger event. The galaxy appears to be relatively isolated in this field.
