The galaxy presents a generally smooth, elongated morphology, appearing cigar-shaped in its overall form. The color profile indicates a concentration of older stellar populations toward the central bulge, exhibiting a yellowish hue. There is little to no evidence of spiral arm structure or significant dust lanes within the galaxy. The light distribution suggests a relatively homogenous stellar population, lacking prominent star-forming regions or intense blue colors typically associated with younger stars. There are subtle irregularities along the edges, perhaps indicating past minor interaction or accretion events. Overall, the galaxy appears to be an evolved system with a well-mixed stellar population and minimal ongoing star formation.
