The galaxy appears as a single, concentrated luminous object. It exhibits a smooth, elliptical morphology, showing minimal evidence of spiral arms or a distinct disk structure. The galaxy's color profile suggests a higher concentration of older stellar populations. There is a notable absence of blue light, which is indicative of recent star formation, supporting the observation of an older stellar population. There does not seem to be any evidence of tidal features or interaction with neighboring galaxies, implying a relatively isolated existence. Overall, the galaxy appears to be a quiescent, early-type galaxy, consistent with an elliptical classification.
