This galaxy exhibits an elongated, cigar-shaped morphology. The light distribution appears smooth and centrally concentrated, indicative of a significant spheroidal component. A faint, extended halo is possibly present, though its boundaries are poorly defined due to the image resolution. There is no evidence of prominent spiral arms or significant dust lanes. The galaxy's overall color is on the redder side, hinting at an older stellar population and subdued star formation activity. The image does not reveal any obvious signs of recent or ongoing merger events, though a subtle asymmetry in the outer regions cannot be entirely ruled out. The galaxy is relatively isolated, with no immediately apparent companion galaxies that would suggest strong gravitational interactions.
