The galaxy appears to be an elliptical type, characterized by a smooth, symmetrical structure with a concentrated central bulge. The light distribution appears to be relatively uniform, with a gradual decrease in intensity from the center outwards. There is no distinct spiral arm structure or obvious dust lanes visible. The galaxy displays a yellowish hue, suggesting a stellar population dominated by older, redder stars. There appears to be no significant sign of ongoing star formation. The overall morphology suggests a relatively evolved system.
