The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with a slight elongation. The light distribution is concentrated towards the center, suggesting a prominent bulge. There is a hint of a disturbed morphology, potentially indicating a past or ongoing minor interaction. The galaxy exhibits a yellowish-red hue, suggestive of an older stellar population with lower levels of star formation activity. The overall shape tends toward being in between round and cigar-shaped. There is evidence of a possible ongoing or past merger event, but the disturbance is relatively minor.