The galaxy presents an elongated, cigar-like morphology. Its central region exhibits a high degree of smoothness, with a dominant yellow-orange hue, suggestive of an older stellar population and potentially a significant dust component. Fainter, bluer patches are observed at the periphery, hinting at regions of more recent star formation. There are no clear signs of a major merger event or strong tidal disturbances. A subtle asymmetry is noted, potentially indicating a minor interaction or internal dynamical processes. Overall, the galaxy appears to be a relatively undisturbed system with a dominant spheroidal component and ongoing, albeit limited, star formation in the outer regions.
