The galaxy presents as a moderately bright, elliptical object. Its core exhibits a pronounced bulge. This bulge has a yellowish-white color, suggesting a population of older stars. 

Extending from the central bulge, a fainter, somewhat elongated disk component is visible. The color of the disk appears slightly bluer than the bulge, implying the presence of younger, hotter stars and potentially some ongoing star formation. 

There appears to be some minor disturbance or irregularity present, or a faint tidal tail. Further spectral data will be needed to determine the dynamics and stellar populations of the galaxy.
