The object appears to be a galaxy, likely a spiral viewed edge-on. It exhibits a smooth, elongated morphology, resembling a cigar shape. A central bulge is visible, displaying a yellowish hue, possibly indicating an older stellar population. The disk component shows a bluer tint, suggesting the presence of younger, hotter stars and ongoing star formation. There is no strong evidence of significant mergers or tidal disturbances, although some minor irregularities may be present upon further inspection. The galaxy's integrated color suggests a moderate level of star formation activity. Its apparent size indicates that it is relatively nearby.
