The galaxy presents as a relatively smooth, single object with a slightly elongated morphology. There is an indication of a brighter, more concentrated core region. Overall, the galaxy exhibits a centrally concentrated light profile, fading gradually towards the edges. The color appears predominantly in the red-green range, suggesting a relatively evolved stellar population, with possible ongoing star formation. No significant spiral arm structure or dust lanes are apparent. The galaxy appears to be relatively isolated, with no clear signs of major mergers or strong tidal interactions. However, there may be some slight asymmetry, potentially indicating a minor disturbance or interaction.
