The galaxy presents as a primarily smooth, lens-shaped structure, elongated with a cigar-like morphology. A central bulge appears concentrated and exhibits a yellow-orange hue, suggesting an older stellar population. Fainter, bluer light is present in the outer regions of the galaxy, indicative of more recent star formation, albeit at a seemingly low rate. No prominent spiral arms or significant dust lanes are immediately discernible. The overall structure suggests minimal interaction or disturbance; any merging activity is likely to be either absent or very minor. The galaxy appears relatively isolated in this field.
