The galaxy presents as an elongated, cigar-shaped structure. It appears relatively smooth, exhibiting a centrally concentrated bulge that transitions gradually into a fainter, extended disk. The central region displays a yellowish hue, suggestive of an older stellar population. The outer regions of the disk show a bluer color profile, possibly indicating the presence of younger, hotter stars and ongoing star formation activity. The galaxy's shape lacks defined spiral arms or prominent dust lanes, suggesting a morphology leaning towards an elliptical or lenticular classification. There's a slight asymmetry in the outer regions which could be due to minor tidal disturbances. Overall, the galaxy seems to be in a relatively quiescent state with moderate star formation.
