The galaxy presents an elongated, cigar-like morphology, appearing as a flattened spheroid rather than a well-defined spiral or elliptical structure. The central region exhibits a brighter, more concentrated luminosity, suggesting a bulge. A subtle color gradient is observable, with the central bulge appearing more yellow/red, indicative of an older stellar population. The outer regions display a bluer tinge, potentially indicating the presence of younger stars or ongoing star formation. There is no clear spiral arm structure visible. No significant signs of tidal disturbances or major merger events are immediately apparent, though a slight asymmetry may indicate minor interactions or recent accretion events. The overall structure suggests a massive galaxy with moderate star formation activity.
