The galaxy presents an overall smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The primary component appears elliptical in shape, with a high degree of central concentration. There is a smaller, slightly irregular component or tidal tail visually connected to the main body, possibly indicative of a past or ongoing minor merger event. Color gradients suggest a relatively old stellar population, predominately redder colors in the center. Evidence of on-going star formation is detectable due to the subtle presence of bluer colors in the main body. Overall, the galaxy is likely to have a significant stellar mass, and low specific star formation rate. The system is at a considerable distance, as evident from the low resolution.
