The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform and symmetrical, with no significant signs of spiral arms or a prominent disk. The galaxy exhibits a predominantly yellow-orange hue, suggesting an older stellar population with a lower rate of ongoing star formation. There is a subtle color gradient from the core outwards, with the central region appearing slightly more yellow, possibly indicating a higher concentration of older stars in the nucleus. There is no obvious evidence of significant tidal interactions or merging events, though a very slight asymmetry in the outer isophotes cannot be ruled out with complete certainty. The overall structure seems to be fairly relaxed and well-defined. 
