The galaxy presents an overall smooth, elongated morphology, indicative of an elliptical or lenticular type. The central region exhibits a concentrated luminosity, appearing brighter and more uniform in color, suggesting an older stellar population dominated by evolved stars. Moving outward from the core, the luminosity decreases gradually with no distinct spiral arm structures visible. The colors appear muted, lacking the strong blue hues often associated with active star formation. The galaxy exhibits a slight cigar shape. There's no obvious evidence of ongoing major mergers or significant tidal disturbances. The apparent smooth structure suggests that it is a relaxed system, likely formed through previous mergers or secular evolution.
