This galaxy presents as a late-type spiral, viewed nearly edge-on. A prominent central bulge is observed, exhibiting a yellowish color, suggestive of an older stellar population. The disk component shows distinct bluer regions, indicating active star formation areas within the spiral arms. The galaxy appears relatively smooth, but there are likely faint, tightly wound spiral arms that are not clearly resolved due to its edge-on orientation and significant distance. No major disturbances or tidal features are apparent, which suggests it is not undergoing a major merger event. However, a very slight asymmetry may be present, meriting closer inspection for minor interactions.
