The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge. The light distribution appears to be relatively even, lacking prominent spiral arms or distinct features. Its overall shape is elongated, suggesting a significant degree of inclination relative to our line of sight, with the apparent major axis being roughly twice the size of the minor axis. The color profile is dominated by warmer tones, indicating a relatively older stellar population and less active star formation. The galaxy does not appear to be undergoing any major merger events or exhibiting significant tidal disturbances.
