The galaxy presents an elliptical morphology. Its overall structure appears smooth, with a high degree of central concentration. A faint, extended halo or envelope is suggested, though indistinct. The color profile is dominated by a yellow-red hue, indicative of an older stellar population and suggesting a lower rate of ongoing star formation. The galaxy exhibits minimal visible signs of tidal disturbances or ongoing merger activity. The roundness of the galaxy is slightly elongated, somewhere in between perfectly round and cigar-shaped.
