The object appears to be a lenticular galaxy at a redshift of approximately 0.044. It exhibits a highly elongated, cigar-like morphology with an apparent lack of distinct spiral arm structures. The galaxy's light profile is smooth and centrally concentrated, indicating an older stellar population. There appears to be a slightly bluer hue towards the outer edges of the galaxy, suggesting some ongoing, albeit low, level of star formation. The light distribution suggests a relatively low Sersic index. Dust lanes are not clearly visible within the galaxy's disk, but it cannot be ruled out entirely. The lack of obvious disturbances indicates the galaxy is not currently undergoing a major merger event. The object possesses a minor axis approximately 0.35 times that of its major axis.
