The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a concentrated, bright yellowish-white luminosity, suggesting a population of older stars. The overall shape appears slightly elongated. A subtle color gradient is observed, with the central regions displaying warmer tones shifting towards cooler, redder hues in the outer regions. There is a slight suggestion of a very faint disk. No prominent spiral arms or significant dust lanes are evident within this image. No signs of major ongoing mergers or tidal disturbances are immediately apparent; the overall structure suggests a relatively settled state.
