The galaxy presents as a single, relatively smooth object with a concentrated central region. The light profile appears to be centrally peaked, indicative of a possible elliptical morphology or a spiral galaxy viewed face-on with a dominant bulge. The color is predominantly yellowish-white in the core, suggesting an older stellar population. There is a slight gradient towards a redder hue in the outer regions, potentially indicative of dust obscuration or a difference in stellar populations as we move away from the center. There is no indication of prominent spiral arms, bars, or significant tidal disturbances. The overall appearance suggests a system that is either passively evolving or undergoing low levels of star formation. The object appears largely undisturbed, with no signs of a major merger or significant interaction with other galaxies.
