The galaxy presents as a diffuse, elongated structure, possibly indicative of a disk galaxy viewed at an oblique angle. There is evidence of a central, slightly brighter region, potentially a galactic bulge or nucleus. The overall color is distinctly blue, suggesting the presence of a young stellar population and ongoing star formation, supported by estimated star formation rates. The morphological classification hints at a system exhibiting disturbances, possibly due to a minor merger or interaction, although smooth features are also present. There is a noticeable deviation from a perfectly smooth elliptical profile, lending credence to the idea it is not a regular elliptical galaxy. The size appears relatively compact; analysis suggests that the galaxy is likely a dwarf galaxy. The presence of disturbed features and blue color is somewhat indicative of a starburst galaxy.
