The galaxy exhibits a generally elliptical morphology. Its color profile suggests a higher concentration of older stellar populations, with a gradual transition to bluer hues in the outer regions, indicating recent or ongoing star formation in a disk structure. The galaxy has a relatively smooth appearance, with no distinct spiral arm structures visible, however the overall morphology is not perfectly smooth, suggesting it is not a perfect elliptical galaxy. There are subtle variations in the light distribution, suggesting either small dust lanes, minor tidal interactions, or potential features of a disk galaxy. The galaxy shows a relatively high central surface brightness that falls off toward the edges. The apparent elongation and position angle of the galaxy are noticeable.
