The galaxy presents as a moderately luminous, elongated structure. It displays a smooth, featureless morphology, with no readily discernible spiral arms or distinct dust lanes. The central region exhibits a concentration of light, appearing more yellow in color, suggesting an older stellar population. The outer regions transition towards a redder hue, possibly indicative of continuing, though diminished, star formation. The overall shape is reminiscent of a flattened spheroid. There is no clear evidence of ongoing major mergers or significant tidal disturbances.
