The galaxy exhibits an elliptical morphology, appearing as a smooth, elongated structure. The core is characterized by a concentrated, bright yellow-orange hue, suggesting a population of older stars. Proceeding outwards from the core, the color shifts gradually to a bluer tint, possibly indicating the presence of younger stellar populations within the galaxy's disk. There is some structural irregularity, as there is a slight distortion or faint arm-like feature present, hinting at a possible past or ongoing interaction with another galaxy, although the disturbance appears minor. The galaxy does not appear to be actively merging with another large structure, though subtle disturbances cannot be ruled out.
