The galaxy presents an elongated, cigar-shaped morphology, suggesting a likely classification as an elliptical galaxy. The light distribution appears relatively smooth, with a concentrated central region that is slightly brighter than the outer regions. There is a noticeable color gradient from the center outwards, transitioning from a yellow-white core to fainter, redder outskirts. This color suggests a potentially older stellar population, with fewer young, massive stars present in the galaxy as a whole. There is no visible dust lane or spiral arm structure. There appears to be a very slight disturbance, which could be due to a small galactic interaction or other environmental effects.
