The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is evidence of a slightly extended halo or disk. The central region exhibits a bright, unresolved core. There may be minimal spiral structure or disk features within the galaxy, though its generally smooth and amorphous shape is likely more indicative of an elliptical classification. Color gradients are present, with a redder hue in the outer regions and a greener tone at the center. This implies a centrally concentrated older stellar population or dust obscuration in the nucleus. The galaxy does not appear to be undergoing any major merging events or significant tidal interactions with other galaxies. Overall, the galaxy seems relatively undisturbed, suggesting an isolated evolutionary path.
