The galaxy presents as a moderately small, relatively smooth, elliptical morphology, appearing as a diffuse central concentration of light. The profile is elongated, exhibiting a cigar shape. There are no readily apparent spiral arms or distinct features that would suggest a disk structure, nor any signs of ongoing major merger activity. A slight color gradient exists, with the central region possibly exhibiting a marginally redder hue than the outer regions. The overall appearance suggests a galaxy with a dominant older stellar population and potentially low current star formation activity.
