The galaxy presents an elliptical morphology, appearing largely smooth and lacking prominent spiral arms. It exhibits a central bulge that appears quite bright and concentrated, displaying a yellowish hue, suggesting an older stellar population dominating this region. The galaxy's overall shape is somewhat elongated, with an aspect ratio suggesting a classification tending towards an E4-E5 on the Hubble sequence. Faint, diffuse bluer regions surround the central bulge, potentially indicating ongoing, but relatively low, star formation within a disk component. No significant tidal distortions or signs of major merger activity are immediately apparent, although there may be some minor disturbances in the outer regions. The overall color profile suggests the galaxy is comprised predominantly of older stars, with a smaller fraction of younger, bluer stars present in the disk.
