The galaxy presents as a relatively smooth and rounded structure. There is a bright, concentrated central bulge that appears nearly circular in projection. The outer regions of the galaxy fade gradually, suggesting a well-mixed stellar population with no distinct spiral arm features visible. The overall color appears to be on the redder end with a yellowish core, suggesting a slightly older stellar population. The light distribution is fairly uniform, lacking strong clumps or knots which would indicate regions of active star formation. There is no evidence of a significant disk structure or dust lanes within the observed image.
