The galaxy presents as an elongated, cigar-shaped object. A central bulge is discernible, exhibiting a yellowish-orange hue, suggesting an older stellar population. Extending from the bulge are faint, bluish structures that appear to be spiral arms or disk-like components. The overall morphology leans towards a smooth distribution of light, although hints of disturbances or faint features are present within the extended disk. The galaxy is relatively compact in size, indicating it may be a smaller galaxy or located at a considerable distance. The color gradient from the central bulge to the outer regions implies ongoing or recent star formation activity in the disk. There is no obvious evidence of a major ongoing merger, though subtle asymmetries might indicate minor interactions in the past.
