The galaxy presents as a relatively small, faint, and elongated object. Its overall shape is suggestive of a highly inclined disk galaxy, viewed nearly edge-on from our perspective. The central bulge, while present, is not particularly prominent, implying that this may not be an early-type spiral galaxy. The disk appears relatively smooth and lacks distinct spiral arm structures, which are difficult to discern given the viewing angle. There may be a slight asymmetry to the galaxy, possibly indicating some minor tidal disturbance or interaction, although this is not a strong feature. The color profile suggests the presence of both older stellar populations, indicated by the redder hues, and potentially some ongoing star formation. Overall, the galaxy appears as a modestly sized and moderately active system at a moderate redshift.
