The galaxy presents a generally smooth appearance, suggesting a relatively featureless morphology. It is primarily elliptical in shape, with an approximate cigar-like elongation. There is a concentration of light towards the center of the galaxy, indicative of a prominent bulge. The galaxy exhibits a color gradient, appearing yellower in the core and subtly bluer towards the outskirts. There is no clear evidence of a prominent disk structure or spiral arms. The overall light distribution suggests an evolved stellar population, with relatively low levels of ongoing star formation. The galaxy appears to be relatively isolated, without any signs of major interaction or ongoing merger events, although minor disturbances cannot be ruled out.
