The galaxy presents as a relatively smooth, elliptical-like structure. Its core appears concentrated and luminous, exhibiting a yellowish-white hue, suggesting an older stellar population and minimal recent star formation activity. The light profile appears to gradually fade into the surrounding space, indicating a lack of distinct spiral arms or a well-defined disk structure. There appears to be a slight asymmetry in the isophotes. There is a small hint of bluer color in the fainter surrounding regions, but these are primarily red and yellow. No apparent signs of ongoing major merger activity or significant tidal disturbances are observed.
