The galaxy presents as an elliptical morphology, appearing largely smooth and rounded with minimal discernible features. The light distribution appears concentrated towards the core, with a noticeable radial gradient suggesting an older stellar population. The color profile indicates a dominant population of evolved stars, with a slightly higher presence of intermediate-age stars in the core, possibly indicating a more recent star formation event there. There is no apparent disk structure, spiral arms, or ongoing major merger activity. Minor disturbances cannot be completely ruled out, but are not obviously indicated.
