The object presents as an elongated, likely edge-on, galaxy. The central bulge appears brighter and yellowish, possibly indicating an older stellar population. Extending outward, there's a fainter disk structure with a slight bluish tint, suggesting the presence of younger, hotter stars. The overall shape is relatively smooth, though subtle irregularities in the outer disk may indicate minor disturbances or interactions. The galaxy exhibits a prominent elongated form, more akin to a cigar-shaped appearance than a perfectly circular one. There's no clear evidence of major mergers or significant tidal tails extending from the galaxy; however, the slight asymmetry might indicate a minor past or ongoing interaction. 
