This galaxy presents as a thin, elongated structure, strongly suggestive of an edge-on spiral or lenticular galaxy. A central bulge region appears somewhat more luminous and exhibits a rounded morphology. The disk appears relatively smooth with no resolved star-forming regions or prominent dust lanes visible in this image. There is no indication of a major merger event in its recent history, although minor asymmetries or faint tidal features cannot be ruled out with certainty given the image quality. Overall, the galaxy appears quiescent, with low levels of current star formation. The estimated diameter is approximately 10 kpc. The colours suggest a relatively evolved stellar population. 
