The galaxy presents an overall elliptical morphology, with the major axis significantly exceeding the minor axis. The central region exhibits a high surface brightness, appearing nearly unresolved and with a concentrated, intensely luminous core. The light profile appears relatively smooth, with no prominent spiral arm structures or distinct star-forming regions immediately apparent. There is a slight hint of a flattened disk component. The color gradient indicates bluer light is present in the inner region, suggestive of a younger stellar population and/or ongoing star formation. The redder light distribution towards the outer edges of the galaxy may indicate an older, redder stellar population dominating the outskirts. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers. Possible minor interaction artifacts cannot be ruled out, evidenced by slight asymmetries in the light distribution.
