The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge that transitions into a fainter, extended halo. The color gradient reveals a yellowish-white core, suggesting a dominant population of older stars. A subtle, blueish color appears towards the outer regions, possibly indicating pockets of younger stars or ongoing low-level star formation. The galaxy lacks any obvious spiral arm structures or prominent dust lanes. There are no indications of major tidal disturbances or recent merger events in the galaxy's overall structure, though there could be a faint hint of a minor disturbance in the halo. The object displays an intermediate degree of roundness, appearing somewhere between fully spherical and highly elongated.
