The galaxy presents a predominantly smooth morphology. Its shape is generally elliptical, appearing quite rounded with a slight elongation. The light distribution suggests a central bulge that is relatively prominent, exhibiting a yellowish-red hue indicative of an older stellar population. This central region is surrounded by a more diffuse, bluish halo, potentially indicating the presence of younger, hotter stars and some ongoing star formation, albeit at a low rate. There is some irregularity in the outer regions, potentially hinting at a past or ongoing minor interaction, or some internal structure.
