The galaxy presents as a lenticular, cigar-shaped system at an approximate distance of redshift 0.146. A dominant, centrally concentrated bulge is apparent, exhibiting a smooth, homogenous luminosity profile. The disk appears highly inclined to our line of sight, manifesting as an elongated structure. Color gradients suggest older stellar populations dominate throughout, especially in the bulge, with a gradual shift towards slightly bluer hues in the outer disk regions. Star formation rate is generally low. No evidence of significant merging or tidal disturbances is observed, with the system appearing relatively isolated and undisturbed. 
