The galaxy presents as a somewhat elongated, disk-like structure. It exhibits a smooth, diffuse appearance, with a central bulge that appears slightly brighter and more concentrated than the outer regions. The light distribution suggests a possible spiral galaxy, but any spiral arms are not well-defined. The dominant colors are yellowish-white in the core, potentially indicating an older stellar population. The outer regions exhibit subtle bluish and greenish tints, which could be attributed to the presence of younger, hotter stars and regions of on-going star formation. Overall, the galaxy displays a relatively even color distribution with no prominent dust lanes or knots of intense star formation immediately apparent. There is no obvious evidence of a major merger event.
