The galaxy presents a generally smooth morphology, appearing as a somewhat elongated spheroid. There is little evidence of prominent spiral arms or a well-defined disk structure. The color profile suggests a population of older stars, with a subtle shift toward the redder end of the spectrum. A faint central concentration of light is observable, but it is not a particularly bright or active galactic nucleus. Minor disturbances within the galaxy's structure are subtly observed, possibly suggesting interaction with another galaxy, however no actual merger is taking place. Overall, it is a relatively quiescent system.