This galaxy presents an elongated, cigar-shaped morphology. The light distribution appears smooth and centrally concentrated, transitioning gradually outwards. There is a subtle color gradient visible, with the core exhibiting a yellowish hue suggesting an older stellar population, while the outer regions show hints of bluer tones, possibly indicative of more recent star formation, albeit at a relatively low rate. There is no evidence of spiral arm structure or significant dust lanes. Overall, the galaxy appears to be a relatively undisturbed system, showing no obvious signs of major merger activity.
