The galaxy presents a generally smooth morphology with a discernible disk-like component. Its overall shape appears elongated, almost cigar-shaped, with a bright, concentrated central bulge. The disk exhibits a moderate degree of disturbance, possibly indicating a minor interaction or recent merger event, although a major merger appears less probable. The color profile suggests a relatively low star formation rate. The redder hues are dominant, particularly within the bulge and inner regions, which may denote an older stellar population with minimal ongoing star formation, compared to the bluer hues in the outer disk. There appears to be a concentration of dust or other obscuring material along the edges of the disk which contributes to the redder colours observed.
