The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge region that gradually fades outward, lacking any distinct spiral arm features. The light distribution suggests an older stellar population dominates, as evidenced by the redder hue, primarily in the central regions. Hints of bluer light are seen sparsely in the outer regions. The galaxy appears undisturbed, showing no signs of major mergers or tidal interactions. The overall shape is somewhat rounded, with no obvious elongation or cigar-like morphology. There are no prominent dust lanes or other indications of significant ongoing star formation. The galaxy appears to be a fairly quiescent system, with a large mass and low star formation rate.
