The galaxy presents as a somewhat elongated, elliptical structure, possibly a spheroid, with a smooth, diffuse light profile. The central region exhibits a slightly higher concentration of luminosity, appearing a bit more yellowish-red compared to the outer regions, suggesting an older stellar population. The outer regions show a gradual fading of light intensity. There is no obvious presence of spiral arms, dust lanes, or significant star-forming regions visible in the image. The overall structure lacks significant irregularities or disturbances, indicating a relatively relaxed or undisturbed morphology. It would be useful to obtain spectra and multi-band photometry for a deeper study of the galaxy.
