The galaxy presents a largely smooth morphology, with a slight elongation from left to right. The galaxy's color profile indicates it is composed of older stellar populations. The central region exhibits a bright, concentrated core, surrounded by a more diffuse halo of light. Evidence suggests a possible ongoing interaction or merger event; a second distinct, though smaller, concentration of light is evident at roughly a 1-2 arcsecond separation on the right side of the primary core. The overall structure is complex and irregular, suggesting morphological disturbance. A faint, extended tidal feature may be present to the right side of the main body, although this is difficult to confirm at this resolution. The roundness of the galaxy is somewhat diminished by the elongated shape of the object.
