The galaxy presents as a relatively smooth, elliptical structure. A distinct central bulge is visible, exhibiting a concentrated, yellowish-white hue, suggesting a high density of older stars. Moving outward from the bulge, the galaxy's color transitions to a bluer shade, indicating the presence of a younger stellar population and potential star formation in the outer regions. No prominent spiral arms or a well-defined disk are apparent; rather, the overall structure appears amorphous with slight irregularities in the outer edges. Faint dust lanes may be present, though their presence is subtle. No significant interaction with neighboring galaxies or tidal tails are readily apparent. The galaxy's morphology is largely undisturbed, with a somewhat rounded, albeit irregular, shape.
