The galaxy presents as a somewhat elliptical, though not perfectly round, structure. It exhibits a relatively smooth overall appearance, but with subtle signs of internal structure. There appears to be a brighter central region, possibly a bulge, that fades gradually outward. Faint indications of spiral arms or tidal disturbances are suspected, but the image resolution makes definitive classification difficult. The galaxy shows a noticeable blue hue, indicating the presence of relatively young, hot stars and ongoing star formation. The color gradient appears consistent, with a slight shift towards redder hues in the central region of the galaxy. There are indications of a possible interaction or minor merger event, given the slightly irregular morphology and subtle wisps that could suggest tidal features. Overall, it is a moderately sized galaxy at a distance determined by its redshift of approximately 0.099.
