The galaxy presents as a mildly elliptical structure, appearing somewhat cigar-shaped. It exhibits a smooth light distribution, with a bright, concentrated central bulge that gradually fades into the outer regions. The color profile suggests a mix of stellar populations, with the central bulge appearing more yellow/white, potentially indicative of older stars, while the outer disk shows hints of bluer hues, possibly indicating younger, hotter stars and regions of ongoing star formation. There is no clear evidence of spiral arm structure or significant dust lanes within the galaxy, suggesting it is likely a relatively evolved system. Overall, the galaxy appears undisturbed, showing no significant signs of ongoing or recent mergers.
