The galaxy presents as a relatively compact object with an apparent high degree of central concentration. The light profile suggests a smooth, elliptical morphology rather than a prominent spiral structure. The color indices, as inferred from the image, indicate a redder hue in the central regions, potentially signifying an older stellar population and/or a higher concentration of dust. Fainter, bluer regions extend from the central body, implying the presence of younger stars or ongoing star formation, albeit at a low rate. There are also subtle signs of tidal disturbances or interactions, visible as faint extensions and asymmetric features around the galaxy, which suggests that it has potentially undergone minor merger events.
