The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region is a bright, yellowish hue, suggesting a population of older stars. The galaxy shows a small amount of flattening. The light distribution indicates that the galaxy lacks prominent spiral arms or a well-defined disk structure. There is a hint of a faint, extended halo or envelope surrounding the main body of the galaxy. A possible faint tidal feature extends from one side of the galaxy, suggesting there may have been a minor interaction with another galaxy. There is a slightly brighter region near the main galaxy, which could be either an area of increased star formation or a smaller satellite galaxy in the process of merging. The color indices suggest a lack of significant ongoing star formation within the main body, while a lower level of star formation is expected given the overall mass estimates.
