The galaxy presents as a relatively smooth, elliptical structure with a noticeable concentration of light toward its center. It appears moderately elongated, exhibiting an axis ratio that suggests a deviation from a perfectly circular form. There is no apparent disk-like structure or spiral arms visible. The color is predominantly yellow-orange, suggesting an older stellar population with fewer young, hot, blue stars, and potential presence of dust. There is no evidence of significant tidal disturbances, major mergers or ongoing star formation based on the smooth texture. The overall impression is that of a well-formed, early-type galaxy nearing the end of its evolutionary process, which is in a relatively quiescent state.
