The galaxy presents a generally smooth morphology, with a dominant central bulge that appears largely spheroidal. The color profile indicates a primarily older stellar population within the bulge, exhibiting a yellowish-red hue. There's a slight asymmetry observed, potentially indicating a minor tidal interaction or past merger event. A faint, extended disk is suspected, discernible as a subtle, greenish-blue glow extending from the central bulge. The disk component, if present, suggests ongoing or recent star formation. Overall, the galaxy appears to be an intermediate to high-mass system, possibly undergoing a transition from a star-forming spiral to a more quiescent elliptical.
