The galaxy exhibits a generally smooth morphology with some discernible features. The overall shape appears to be somewhat elliptical but trending to cigar shaped. The light distribution suggests a substantial central bulge, with a notable decline in surface brightness towards the outer regions. There is a complex arrangement of features, suggestive of an interaction with another galaxy. Star formation appears low, mostly in the center of the bulge. There are some irregularities present, which may indicate a mild state of disturbance, possibly a minor merger event. The color indices suggest the presence of an older stellar population.
