The galaxy presents as a relatively compact object with a notable central concentration of light. Its morphology appears largely smooth, lacking the obvious spiral arms or irregular features indicative of disk galaxies or major mergers. There is, however, a slight elongation or subtle asymmetry that could suggest either a minor disturbance, ongoing accretion, or a subtle disk component oriented close to edge-on. The color profile is somewhat uniform, with a generally bluish hue concentrated in the central region of the galaxy, possibly indicating active star formation. The outskirts of the galaxy appear fuzzier and redder, which could be suggestive of an older stellar population dominating the outer regions. No significant tidal features or shells are immediately apparent. The overall appearance suggests a galaxy that is somewhere between a quiescent elliptical and a disk system experiencing low levels of activity.
