The galaxy presents as a roughly circular, smooth object with a concentrated central region. The color profile indicates a relatively blue core, which transitions to a redder hue in the outer regions of the galaxy. This color gradient may suggest a difference in stellar populations, with younger, hotter stars dominating the central region and older, cooler stars more prevalent in the galaxy's outskirts. The smooth texture implies a lack of significant dust lanes or spiral arm structures. There is no prominent central bulge apparent, and the galaxy's overall structure appears undisturbed, showing no obvious signs of interaction or recent merger activity. Marginal disturbances may be indicated by small, faint tidal features.
