The galaxy presents as a somewhat elliptical, diffuse object with a central bulge that appears brighter and more concentrated than the surrounding disk. The color profile suggests a mixed stellar population. The central bulge exhibits a yellowish-white hue, indicative of older, redder stars. The outer regions of the galaxy display a bluer tinge, possibly suggesting the presence of younger, hotter stars and ongoing star formation. Faint, extended arms are suggested, though not clearly defined. There is some indication of minor tidal disruption, but no clear signs of a major merger event. The galaxy appears to be a relatively smooth system, with no significant dust lanes or prominent star-forming regions clearly visible in this image.
