This galaxy presents as a largely smooth, elliptical-type structure with a concentrated central bulge. The color profile indicates a primarily older stellar population, exhibiting a yellowish-orange hue. There is little evidence of significant dust lanes or spiral arm structures. The galaxy appears to be relatively isolated, showing no immediate signs of major tidal disturbances or ongoing mergers, with the exception of a possible minor disturbance, though this may be an artifact. The morphology suggests a system approaching quiescence, with a low rate of star formation. Its shape is mostly round with hints of being somewhat in between round and cigar-shaped.
