The galaxy presents as a moderately luminous object with a concentrated central bulge and a slightly elongated, elliptical morphology. The core appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue. There is a hint of a fainter disk component surrounding the central bulge, though it is not well-defined.  There are subtle indications of minor disturbances in the galaxy's overall shape, possibly hinting at ongoing or past interactions.  The galaxy appears to be undergoing a relatively low rate of star formation.
