The galaxy presents as a fairly smooth, elliptical-like structure. There is a concentrated central bulge that appears a yellowish-white color, indicating a population of older stars. Moving outward from the core, the light becomes less concentrated and more diffuse, fading into the background. There is a subtle blueish tinge to the outer edges of the galaxy, implying some level of ongoing star formation, although likely at a low rate. The shape is mostly round with a hint of being in-between round and elliptical. There's no strong visual evidence of spiral arms or a well-defined disk structure. No significant signs of major merging or tidal disturbances are apparent, only a minor disturbance.
