The object presents as a lenticular galaxy, exhibiting a smooth, elliptical morphology with a high degree of central concentration. The light distribution appears relatively even, suggesting an older stellar population. I observe a distinct lack of spiral arm structure or prominent dust lanes. The galaxy is elongated, with a cigar-like shape, indicating it is viewed edge-on or at a high inclination angle. There are no signs of any major ongoing merging events or tidal disturbances. A faint blue tinge is present within the central regions, hinting at some, albeit weak, ongoing star formation. Overall, this galaxy seems to be a relatively undisturbed system, likely a passively evolving galaxy.
