The galaxy presents a predominantly smooth morphology. The central region exhibits a bright, yellowish-white core, indicative of a high concentration of older stars. Surrounding this core is a more diffuse halo with a slight blueish hue, potentially suggesting some ongoing star formation, albeit at a relatively low rate. The overall shape appears somewhat elliptical, with a moderate degree of elongation. There are subtle hints of internal structure, such as faint irregularities in the outer regions, but no distinct spiral arms or bar features are apparent. The galaxy's appearance is consistent with an intermediate-mass system, likely a late-type lenticular or early-type spiral galaxy viewed at a significant distance. There is no visually obvious evidence of any major ongoing merger activity, though some minor disturbance within the extended halo cannot be ruled out. The galaxy seems to have a substantial mass that does not inhibit a degree of star formation.
