This galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The galaxy exhibits a generally elliptical shape, appearing mostly round with a slight deviation from perfect circularity. The color profile is dominated by redder hues, suggesting a stellar population that is relatively old and evolved, with diminished ongoing star formation. There are no prominent spiral arm structures or significant dust lanes visible. There may be evidence of minor disturbances or interactions with another galaxy in the recent past. The overall appearance suggests a galaxy with a substantial stellar mass.
