The galaxy presents as a slightly inclined disk system with an approximate effective radius of 9.7 kpc. It exhibits a smooth appearance, hinting at an older stellar population, although there are faint hints of blue regions which may suggest pockets of younger stars. Its overall form is elongated, nearing cigar-shaped, with a bright central bulge dominating its luminosity. There are no distinct signs of strong spiral arms. The galaxy exhibits a low level of disturbance, with no signs of ongoing major merger activity. Star formation is present, with average specific star formation rate around -10.35, suggesting it is relatively quiescent, but not completely inactive.