The galaxy exhibits a predominantly smooth, elliptical morphology. It is characterized by a concentrated central bulge that gradually fades into an extended halo. The light distribution suggests a relatively old stellar population, with a yellowish hue dominating the overall color. There is little evidence of spiral arm structure or significant dust lanes, indicating a lack of ongoing major star formation activity. The galaxy appears relatively undisturbed, lacking strong signs of recent merger events or tidal interactions.
