The galaxy presents as a somewhat elliptical structure with a brighter, more concentrated central region indicative of a bulge. A flattened disk component is subtly observed, suggesting a classification leaning towards lenticular. The color profile suggests a higher concentration of older stellar populations, as evidenced by the reddish hue of the bulge. Star formation appears to be suppressed, potentially indicating the depletion of gas reserves. There is no significant evidence of ongoing mergers or major tidal disturbances, suggesting it is a relatively undisturbed system. Overall the galaxy appears to be a massive, evolved system that has largely exhausted its star-forming fuel.
